David's Astronomy Pages
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![]() Notes (S1302) |
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![]() Notes (S1304) |
Main aims
Equipment & Software
Highlights
Summary Plots & Logs
Observing Plan![]() |
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Observing Result |
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Dome & Scope Slewing Performance | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Slew/Centering Performance | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Guiding Performance | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Sky Conditions (Locate Frames) | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Night Sky Summary Plot Top axis: Sky Brightness at Zenith (in ADU/s) Lefthand axis: Local Time (hh LT). Righthand axis: Sun Altitude (degs) |
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Actual Weather vs Pre-Session Weather Forecast | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Session Event Log | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Session Alerts & Alarms | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Back to Top
Fig 1. Foc2 Focus Profile (wide)
Fig 2. Foc2 Focus Profile which was rejected due to "Quadratic values indicate poor/invalid profile"
Back to Top
A Geomagnetic Monitoring Station is being added to the Observatory in
Spring 2025 for
monitoring changes in the earth's magnetic field and to supplement and build
upon the Observatory's existing Aurora monitoring using AllSky Camera and
new NorthCam Camera.
Earlier notes regarding selection of SAM III System
are covered in:
Review -
Potential Geomagnetic Monitoring Station (2025-01-24)
SAM III Order arrived today (2025-03-18) and installation plan is being
developed.
Questions:
Q. How are cable wires fitted to the SAM III Controller Box.
A.
Bared ends of wires are inserted into appropriate slots in the green
10-position pluggable terminal block X2. , and screws tightened.
After double checking that correct wires are in their correct slots, insert
green adapter bars in port on SAM III controller box
1 GND X
2 Signal X
3 +5Vdc X
4
GBD Y
5 Signal Y
6 +5Vdc Y
7 GBD Y
8 Signal Y
9 +5Vdc
Y
10 Not used.
Q. Identifying Cables to/from Sensor Sensors ?
Three CAT6 cables should
be clearly identified at both ends, marked X, Y, Z according to which
axis they will each be connected to.
Q. A standard 'scheme' should be defined to detail the particular
wires in the CAT6 cable that will be used for connecting to the GND, OUT and VCC pins
on the FG-3+ sensors and to the relevant slots on the Controller Box.
GND - Blue Wire = Ground
OUT - Orange Wire = Sensor
output
VCC - Brown Wire = +5 V Power
Q. How to ensure that water can't enter to the Piped Sensor Unit at
the point of cable entry. (3 Cat6 cables and 1 temperature cable)
A.
Inverted U Tube ?, Expoxy Filler,
Q. How to build 'cage' for mounting the
three FG-3+ sensors.
A. Circular Wood Cage ? , 3D
Printed Cages from Torc ?,
Q. How to wire up the FG-3+ sensors
(including 10 µF, 25 V tantalum
capacitor & 100 nF 25 V multi-layer ceramic capacitor ) ?
A. Refer to wiring plan in manual
Q.
How to connect wires
to 3 pin adapter using metal tags. How are the metal tag inserted into
plastic adapter ?
A. From Installation Guide:
A 3-pin
single inline header connector and contacts are supplied for connecting
cable to each sensor. Crimp or solder the sensor cable wires to the contacts
and insert them in the SIL header connector. The SIL header connector has
slots on one side, and the tiny tabs on the contacts must be inserted on
this side. Do not solder wires directly to the sensor. The sensor pinout is
indicated on the sensor label and in the drawings below.
The socket
contacts require a double-crimp, one for the conductor and one for the
insulation. If you do not have a crimping tool and must solder the wires, it
is suggested you cut the insulation crimp fingers off of the contact
(otherwise, it is unlikely you can fold the fingers enough to make them fit
the header connector). You will need to fold the conductor crimp with a pair
of miniature pliers. Do this very carefully to avoid damaging the contact.
Apply a very small amount of solder – if you apply too much solder it will
wick up into the socket.
Before inserting the single inline (SIL)
header onto the sensor pins, put a small amount of dielectric grease (for
example, Permatex 81150 available at most automotive parts stores) on the
sensor pins. The amount of grease used should be small enough that it is not
visible on the pins. This will help prevent corrosion if the sensor is used
in outdoor applications. The header has no built-in polarity indicator so it
should be marked with nail polish, paint or tape to indicate proper
orientation.
Q. Does the existing 12mm Male Plug from the A/C Power Adapter Unit
need to be replaced with either the longer 14mm plug or with 12mm plug with
locking nut. ?
A. Controller Unit was tested with existing 12mm
Male Plug and it initialises ok. A disconnection/reconnection occurs
if the plug is physically rotated, but not under general use. It seems
secure enough.
( I'd rather not change the plug as this requires cutting
off the existing male plug and soldering/crimping wires to the new plug and
then rely on screwed connection on working loose.)
Q. How should the X, Y & Z Geomagnetometer Sensors be orientated
?
A. As per construction manual
X
North-South , pins SOUTH
Y
East-West, pins WEST
Z Vertical,
pins UP
Q. What entries should be made in the SAM_VIEW setup/settings ?
A. Settings
Owner or Station Name :
Clair Observatory
Location :
Ellon, Scotland
Longitude, Latitude
02.00W, 57.32N
IARU-Locator :
IO87xh
Q. What are expected 3-axis field strengths ?
A.
Using the calculator at
World Magnetic Model 2025 Calculator (geomag.bgs.ac.uk) the expected
field strengths at the Observatory for 2025-04-01.
X:
16467nT (4.4 nT/year)
Y:
-100 nT (59.1 nT/year)
Z: 47326 nT (32.8 nT/year)
H : 16468 nT (4.0 nT/year) (Horizontal
Intensity, from X & Y vector sum)
F : 50110
nT (32.3 nT/year) (Total
Intensity)
D : -0.348 deg East
(12.4 arc min/year)
I : 70.814 deg
Incl'n (0.5 arc min/year) ' Angle from Horizontal
- See
also
What are the
geomagnetic components ? (intermagnet.org)
Q. What is the geomagnetic latitude of the Station
A.
54.36° N
From IGRF, At Epoch 2025.0 Lat 57.32 N, Long -2.00 E, the
Quasi-Dipole Latitude is 53.36° (vs Dipole Latitude 59.26°)
Update 2025-03-19 (SAM III - PC Connection)
- Created program folder 'C:\More Programs\SAM'
and copy into the folder the files from
'..\Software-Firmware\SAM3 Applications'
'..\Software-Firmware\Runtime Libraries'
- Installed SABRENT USB-Serial Driver
. CD ..
/Windows/PL23XX_Prolific_DriverInstaller_v301-WIN11/PL23XX-M_LogoDriver_Setup_v301_20211221.exe
- Used PL23XX_checkChipVersion_v1020.exe' to check
'COM4' this gave the meessage :
"This is a PL-2303 GS chip"
- Made a trial connection to SAM III unit
- Connect USB-Serial
Cable to Computer
- Appears as "Prolific PL2303GS USB Serial Com
Port (COM4)
(COM4 on Development/Analysis Computer)
- Connect USB-Serial Cable
between Computer and SAM III box via Serial Pass Through Cable)
- Opened SAM_INI_v2-0.exe
- Selected COM Port (COM 4)
- Set default
values used to confirm values on Form are defaults.
(proven by
changing a value and then using Set Default Values to see it overwrite the
manually changed value)
- Tried 'Send parameters'.
After running to 100%, 'Error!' dialog shown with message "Error while
writing parameter set!"
Tried 'Receive parameters'
After running to 100%, 'Error!' dialog shown with message "Error while
reading parameter set!"
A Port Monitor confirms that data
is coming from the SAM Unit with data every second, like
20.03.25
15:57:01: X,,Y,,Z,
-If SAM_INI_v2.0 is opened and connected to COM4 with the SAM III in
command mode (F1) and
'Send Parameters' is used, SAM_INI runs to c. 50%
and then displays message "SAM does not respond".
- Trying again :
'Receive
Parameters' , trackbar runs to 100% and message 'Parameter read
successful.." appears
Trying again
'Send Parameters' :
trackbar runs to 100% and message 'Parameter write successful.."
appears
After a successful 'Write', the SAM box
automatically resets itself.
To do:
- Dig a 120 cm deep hole to contain 3-axis
geomagnetometer sensor fixture (see Update 2025-03-23 to
Updates 2025-03-25 below)
- Prepare 3 CAT6 cables, one cable for each sensor
- Prepare Temperature Monitor (see
DS18B20 Waterproof Digital Temperature Sensor (2025-03-19)
Update 2025-03-23 (Hole)
Hole that will contain the
3-axis geomagnetometer sensor fixture has been commenced on 2025-03-21 and
reached 45 cm depth. Pictures below show status of hole on 2025-03-23
after reaching 68cm.
Update 2025-03-24 (Hole)
Hole that will contain the
3-axis geomagnetometer sensor fixture has now
reached 100cm depth. Another 20cm to go
Update 2025-03-25 (Hole)
Hole that will contain the
3-axis geomagnetometer sensor fixture has been completed after reaching
120cm depth.
Completed Hole for the 3-axis geomagnetometer sensor fixture Hole depth is 120cm |
Detailed image showing lower part of hole | |
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Side view of hole 120cm depth |
Side view of hole 120cm depth. |
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Sensor | Circuit | Sensor Orientation | |||
North (X) | East (Y) | Down (Z) | |||
Magnetometer 1 | Circuit A (x) | ||||
Circuit B (y) | |||||
Circuit C (z) | |||||
Magnetometer 2 | Circuit A (x) | ||||
Circuit B (y) | |||||
Circuit C (z) | |||||
Magnetometer 3 | Circuit A (x) | ||||
Circuit B (y) | |||||
Circuit C (z) | |||||
Expected Values | 16467 | -100 | 47326 | ||
(BGS 2025 Model) |
Update 2025-03-30
Calculated required Magnetometer
Offsets to sensors
X -833 Y +13584
Z+11815
Using -82000 + required offset we get
X -82833,
Y -68416 Z -70185
These were applied to SAM
unit via SAM Init
Update 2025-04-02 (System Burn-In)
A 72 hour
'burn-in' has been commenced on the workbench (aka dining room table) with
sensors hooked up to SAM III Unit and PC. This is too check that everything
is working reliably and there are no failures of any of the components
(better to find out something now than after the fixture is buried !).
The Burn-In period will allow Bx, By, Bz readings to be followed in an
attempt to understand the cause and effect of any deviations seen in the
readings
Update 2025-04-02 (Sensor sensitivity)
A 72 hour
'burn-in' has been successfully completed. System working throughout
period, though not connected to the PC for the entire period.
The
magnetograms show that the sensors are very sensitive to temperature, which
is of no surprise given the relativey large temperature coefficient of the
sensors (between -100 & -150nT/°C), the fact that sensors are not insulated
and are subject to various daily changes to temperatures and to central
heating cycles.
The sensors are also demonstrated to be
very sensitive to any small or larger movement of the sensor.
Other
effects such as changes to ferro-magnetic environment caused by a car on the
driveway (10m) or a new skip / moving wheelbarrows on the estate road (20m)
are detectable but cause much lower deviations to magnetometer readings than
temperature/precise position & orientation do.
During the 72 hour
burn in there was geomagnetic changes (noted by the presence of viewable
aurora and Scandinavian magnetometers deviations), but these effects (the
signal) is much smaller than the other changes (especially temperature)
Noise due to i) thermal effects, ii) movements of the
magnetometer sensors, iii) changes in large ferro-magnetic objects in
front of the house will be largely eliminated by enclosure in magnetometer
fixture assembly and by burial in the rear garden to a depth of at least
80cm below ground surface.
Whitham Reeve has looked at the
Magnetometers (2025-04-06) and beside the recommendation to continue the
tests for longer to fully appreciate the cause and effect from different
factors, he considers that the magnetogram traces look normal for the test
conditions described and that there is nothing fundamentally holding me from
final assembly of sensor fixture and its burial.
Update
2025-04-07 (Extended Monitoring)
Monitoring was continued
the following day
Update 2025-04-08 (Temperature Relationships)
A
14 hour test was run during during which magnetometer sensor positioning was
stable (no knocks or changes etc) and temperature monitoring running. The
test occured through a time interval in which the central heating
(thermostat in an adjacent room) is automatically turned down to 16°C
at 21:30 UT, turned up to 20°C at 07:00 UT, and turned slightly down to 19°C
at 08:30 UT, producing a nearly 4°C change in ambient room temperature.
Data was compiled using AstroMag (a custom application that read the
SAM III data file and the DS18B20 temperature sensor) and then plotted in Excel.
The following chart
shows the changes in Bx, By, Bz and Bh (blue, red, green & magenta lines)
from the point that the run commenced, Temperature (black line), and the
modelled magnetometer change based on temperature coefficients of 100 nT/°C
and 150 nT/°C (dashed line).
The Central Heating Controller (thermostat located in an adjacent room)
is set to reduce thermostat threshold turns down to 16°C at 21:30
UT, turns up to 20°C at 07:00 UT, and turns slightly down to 19°C at 08:30
UT. This effectively means that radiator heating is off during
the chart period 22:00 to 07:00 and then on again at 07:00 to around 09:00
or so. During this time there is around a nearly 4°C change in
ambient room temperature. Minimum outdoor temperature during the night was
1°C ( It is possible that there is some central heating
between 06:30 and 07:00 dependant on the temperature in the adjacent room
(c. +/- 16°C). It is also possible that the workbench room begins to
stabilise in temperature at this time due to daytime solar radiation from
outdoors)
The setup used during the test is shown in the
following photo. The 3 magnetometer sensors are all located together (within
30cm of each other) at a distance of around 2.2m from the room's radiator
and around 1.4m from the room's window.
The graph above shows a firm (inverse) relationship between Magnetometer
Change and Temperature.
However it is unclear why
i) the Y
sensor shows a significantly stronger relationship to temperature than that
expected (based on the published -100 to -150 nT/°C coefficient range), and
ii) the X sensor shows a significantly weaker relationship to
temperature than that expected.
- Do the 3 sensors have a
significantly greater range in temperature coefficient than the 'published'
range
- Does the self-built circuitry associated with each sensor cause
the wider variation ?
I'm a poor amateur at soldering (I'm too
embarrassed to show the photos here!). Whilst the circuits all work, I've
almost certainly used more solder than an expert would. I purposely applied
solder to both upper and low sides of the mini-boards (to minimise chance
that any one solder join fails through the life-time of the Station). The
precise distances between the circuit and the sensor is slightly different
between the 3 builds (e.g. 4.5 cm for X , 5.5cm for Y) and there are
potentially other small points of difference on the 3 boards. Whilst the
capacitors are all in the correct place in a circuit sense and the (longer)
pin of the tantalum capacitor is in the correct "+" position on all the 3
boards, the height at which I have the tantalum capacitor mounted above the
board varies (due to my poor skill level). For the X Sensor Circuit it is
mounted close to the board but in the Y sensor Circuit it is mounted around
6mm higher than for X. Ideally I would have constructed all the circuits to
be precisely identical but I was learning as I was going using a new
(digital controlled) solder iron. With tiny boards one really needs 4
hands (one to hold the soldering iron, one to hold the solder wire , one to
hold board and one to hold the electrical wire or component !) Q. Can any
of this explain the difference in Temperature Coefficients ?
Earlier
tests using each sensor with each circuit in turn and in each of the 3
orientations was inconclusive regarding the impact of the each circuit. This
was due to the precise effect of sensor positioning and the large thermal
effects). Those tests did show that each sensor needed a significantly
different offset to bring its readings in line with those expected for my
location.
In the final installation where thermal
variations will be much smaller, differences in the temperature coefficient
between the 3 sensors (including self-built circuit) will be much less
important. However if there are strong differences in the
sensitvity/responses of the 3 sensors to non-thermal magnetic changes that
is of more concern.
The recorded magnetometer values during the same
time period are shown in the chart below:
These compare with expected readings at the Observatory location of
X: 16467nT , Y: -100 nT ,
Z: 47326 nT , H : 16468 nT
These include
following offsets from raw (-82000 based values) :
X -833
Y +13584 Z+11815
Note : These offsets will be
updated again once sensor fixture is installed & buried at final site.
Update 2025-04-09 (Sensors)
Based on the Sensor2's higher sensitivity to temperature changes (Y in
above burn-in & monitoring tests) it has been decided to use it as the Z
Axis Sensor. This means it will lie deepest of the 3 sensors and can
be expected to experience the least temperature fluctuations.
As a
consequence Sensor3 (Z in above burn-in & monitoring test) will be used as
the Y Axis Sensor
Sensor1 will continue as the Z Axis Sensor
The sensor cables have been re-coded with coloured electrical tape at
both ends for identification
X Axis (Sensor1 / CableA) -
Blue
Y Axis (Sensor3 / CableC) - Red
Z Axis (Sensor2 / CableB)
- Green
Began assembly but ran into problems with
i) a couple of wire to
3-pin terminal breaking (at circut board end and/or terminal end)
requiring resoldering,
ii) the 3 socket plastic terminal coming loose
from SG-3+1 pins when trying to work the circuit board into place in the
Side-Elbow Junction.
One of them was eventually reinserted but in
the other case
iii) the blue wire to the Y Axis Sensor broke again and
the after reattaching to the terminal socket it was found that
iv) the
socket could not be inserted far enough into the terminal so that
v) a
reliable connection to the SG-3+ GND Pin couldn't be archieved
May need to buy some new pipework for housing the Y axis Sensor (End Piece, Straight Junction and Side-Elbow Junction.)
Update 2025-04-10 (Sensors, Assembly)
New End
Piece, Straight Junction and Side-Elbow Junction bought from Hardware Shop
in order to replace the housing that had to be sacrificed to get the FG-3+
sensor out in order to reconnect it again.
New housing
successfuly built.
Assembly commenced with building/assembly of
Y and Z housing.
Update 2025-04-11 (Assembly)
Assembly of
magnetometer sensor fixture completed including Temperature Sensor Probe.
Cable inlet sealed with two plugs of Epoxy Fller
Update 2025-04-12 (Installation Prep)
- External surface of pipe joints and the cable inlet/filler have now been
double coated with PVC solvent glue.
- Cables have been bound into a
cable bundle, and threaded through the flexible pipe. There was too
much friction/ bend to allow the cable to be passed through the entire 10.5m
flexible cable in one go and it decided to cut the flexible pipe into 4
pieces to allow the cable bundle to be successfully passed through.
- The middle shelf in the Observatory Computing Bay has been cleared in
preparation for placing the SAM III unit on. Lower shelf is confirmed to be
loosely position which will allow it to be temporarily removed for drilling
hole in floor of the Observatory Computing Bay for pulling through the cable
bundle from the Magnetometer Sensor fixture.
Update 2025-04-13 (Installation)
- Hole has been marginally deepened (in the area of the Z Axis Sensor) to
allow the entire Sensor Fixture to be placed as deeply as possible.
- A trench between the Sensor Hole and the Observatory has been dug for
taking the flexible corregated pipe which contains the cable bundle from
Magnetometer Sensor fixture.
- Flexible Pipe / Cable Bundle have been laid back
to the Observatory, and cable bundle passed through hole into the
Observatory.
- Flexible Pipe backed away from Observatory, and breaks
between Pipe Sections joined with tape.
- Trench back filled and lawn
repaired.
- Ardunio connected to Lindy USB Hub (in Observatory Computing Bay) - Appears as COM8 in DeviceManager
- AstroMag modified to use COM8 as default port for Temperature Data and issued as AstroMag 1.2.1
- Sabrent USB-Serial Convertor Driver installed on Observatory Computer
C:/Data/Computer/Home Computers/SABRENT USB-Serial Converter
Driver/Windows/PL23XX_Prolific_DriverInstaller_v208/PL23XX-M_LogoDriver_Setup_v208_20211221.exe
- SAM III connected - Appears as COM9 in
DeviceManager
Update 2025-04-14 (Installation)
- Sensor Cables tied into SAM III Unit and Ardunio Project Box, using
existing wire ends
(cables still need to be trimmed back to an
optimal and equal length)
- Confirmed that signals are being received, and that SAM_VIEW and AstroMag are working
- Sensor Fixture has been installed in
the Hole, oriented N-S , E-W & Vertical, half buried
- Last 1m of cable bundle has been buried at
depth in the hole
- Hole back filled and
lawn repaired
- Sensor Hole geolocated to allow the Sensor Fixture to be
recovered in future, should it be required
- Sensor signals monitored for stabilisation
Sensor Fixture sitting at bottom of hole Picture taken prior to alignment |
Sensor Fixture at bottom of hole (detail) shows 1m length of cable bundle that will be buried at same depth as the sensor also shows North-South axis (blue), East-West Axis (red) and Vertical Axis (green, at bottom of hole) |
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Setting up North-South Survey Line This was done by creating a line parallel to Observatory's North-South Alignment Picture is looking Due North along string line (see Observatory N-S Alignment, 2018) |
Sensor Unit Positioned according to Survey Line Unit positioned vertically, centred on the North-South Survey String, and with X Axis aligned with the North-South Survey String 4 canes pushed into the bottom of hole hold the Sensor Unit in position pending burial |
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Sensor Unit Alignment Due to location of sensor at bottom of hole its alignment had to be done by eye. |
Sensor Unit in Finalised Position ready for burial |
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Sensor Unit being buried Z & Y Sensor Axes have been buried at this point |
Sensor Unit being buried All 3 sensor axes and cable inlet have been buried at this point. Just the top of the sensor unit is visible Hole was subsequently back filled up to the level of the lawn |
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Update 2025-04-15 (Analysis / Potential Calibration)
Magnetograms from 1st day (2025-04-14) plotted and analysed.
First
plot shows readings from the morning and early afternoon from time that Sam
III unit was powered up with the Sensor Fixture positioned in the 1.2m deep
hole, but not yet fully aligned and not yet buried. Data trends are
consistent with a negative relationship to temperature. Data is quite
noisey. Would there be a benefit in using moving averages ? (or
average the 10s samples to create a 1 min binned average).
X | Y | Z | |||
Expected Values | 16467 | -100 | 47326 | ||
Prior Fixes | -833 | +13584 | +11815 | ||
Currently used offsets | -82833 | -68416 | -70185 | ||
Current Av Values | 21540 | 13280 | 45030 | ||
Additional Fixes | -5083 | -13380 | +2296 | ||
Proposed New offsets | -87916 | -81796 | -67889 |
Update 2025-04-16 (Analysis & Diagnostics)
- Some issues occuring with AstroMag encountering with exceptions which
causes SamMonitor loop to exit, which stops data recording.
Fixed in
AstroMag 1.2.5.
- Spiky temperature values that started the day before was in partly due to temperature values being sampled every 60s for graphing. A more valid and smoother temperature is producing by averaging temperature values (that are read every1s) over a 60s window.
- Anomalous jumps in Y reading are still occuring (eg. an anomalous -283 nT shift in Y reading at 2025-04-16 11:50 UT that was proceeded by an anomalouus +1400nT spike). This is ranked a Major Issue.
- Began some diagnostics tests that aim to understand high noise levels,
but might cast some light on the Sensor Shift issue. The first test
which was to turn-off the power to the Temperature Sensor at 13:23 UT which
showed an immediate and significant downward shift in all 3 sensor reading ,
with X,Y, Z readings shifting by -716nT, -548nT & -454 nT
respectively.
- It was hoped that running the station with the Temperature Sensor
turned off would fix the issue with anomalous shifts in Y reading with
associated smaller shifts in X and/or Z reading, however after around 5
hours the problems with shifts in Y reading resumed again.
Update 2025-04-17 (Further Diagnostic Testing)
- As part of continued testing SAM III Unit was turned off in order to disconnect the Y Magnetometer and to see if this would eliminate anomalous shifts in readings. Obviously the Y readings (which have shown the biggest shifts) won't be now available, but it is hoped to tell if smaller shifts in X & Z readings continue or not. After a delay of 15 minutes of so the SAM III unit was restarted and data log resumed. Piecing together data it would seem that after turning on the X and Z Magnetometers (without the Y Magnetometer running) saw an upward shift in X and Z readings of +400 and +100 respectively. The net shift gradually reduced to +350 and +50 after 1 hour.
Update 2025-04-18 (Further Observation)
- Some 25 hours of observations have been completed with the Y Axis Magnetometer turned-off and there have been no anomalous shifts during this time
- Data Readings are still rather noisy and with, as yet, no definate explanation or cure.
- The noise can be cleaned up using a 7 min moving average (averaging
data +/- 3 mins of the plotted time point), and this highlights the key
trends in the data which are of geomagnetic origin.
- The geomagnetic origin is highlighted by the following comparison of the X Axis magnetometer readings and a stackplot of Scandinavian magnetograms. The X Axis Magnetometer appears to show deviations that are twice as large as those shown by dob-sol-kar stations. This isn't understood. Is the scale bar on the mkstackplot being misunderstood ?
- Downhole Temperature Monitoring has been turned back on at 13:20 (12:20
UT) in order to understand its effect on X & Z magnetometers, beyond the
expected initial shift in readings. Provide the shift is remains static it
is manageable.
The magnetogram (below) shows there was a +370 nT
shift in X Axis Readings and a +498 nT shift in Z Axis Readings when the
Temperature Sensor was turned on. These compare with the earlier
shifts of -716nT and -454 nT
respectively when the Temperature Sensor was turned off two days earlier
(2025-04-16 14:23 (13:23 UT).)
During the first 6 hours with Temperature Sensor running there have been
no anomalous shifts in X & Z readings
This would seem to point to the
Y Axis Magnetometer as being the cause of the random large shifts in
magnetometer readings.
2025-04-18 (Remedial Plan)
It seems that the Y
Axis Magnetometer is compromised in some way.
Rather than dig up the
existing 3-axis Sensor Fixture and pull out the working X & Z sensors and
build into a new 3-axis fixture using a new Y axis magnetometer, it is
proposed to build a dedicated Y axis fixture for setting beside the existing
fixture.
Requires
- new FG-3+ magnetometer (£67.70 from
https://robosavvy.co.uk/fgsensors-fg-3-sensor.html)
- new
fluxgate capacitors
10 uF, 25v Tatalum
Capacitor (£ 1 + delivery_
100 nF, 25v
Ceramic Capacitor (£ 1 +delivery)
- new piping (3 ends caps, 1 x 90
deg bend, 1 x 135 deg bend, 2 connectors - £10)
- new 15m length of Cat6
cable required (already available)
Work
Assembly / test new magnetometer &
fixture
Part dig existing hole, install new Y Axis fixture
Dig up trench, thread new cablethrough corrugated pipe (if possible)
or run cable beside corrugated piper
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This Web Page: | Notes - Session 1303 (2025-03-18) |
Last Updated : | 2025-04-18 |
Site Owner : | David Richards |
Home Page : | David's Astronomy Web Site |