geomagpy / magpy

MagPy (or GeomagPy) is a Python package for analysing and displaying geomagnetic data.
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Missing export to IBFV2.00 INTERMAGNET Baseline Format #126

Open mlnorthernswe opened 1 year ago

mlnorthernswe commented 1 year ago

I can't see how I can get IBFV2.00 file that is used in INTERMAGNET yearly DVD: https://www.intermagnet.org/data-donnee/formats/ibfv200-eng.php It should be suitable to create that file when exporting to IAF format as those files are used in mentioned INTERMAGNET yearly DVD. The README.IMO file is created already when exporting to IAF. Also https://www.intermagnet.org/data-donnee/formats/iyfv101-eng.php should also be created when exporting to IAF as that file is also used in the INTERMAGNET yearly DVD.

leonro commented 1 year ago

Both files can be created using MagPy. They are not created automatically as they are based on different sources (Di values plus adopted baseline, BLV) or require a distinct coverage (IYFV).

Regarding IYFV

When i.e. IAF exports are finished or any other data file containing one year of one-minute data is available: Open the full year of one-minute data - got to menu file -> export. Within the "export" window select an appropriate directory and choose the "IYVF" format from the dropdown menu. Do NOT change any further export options. The suggested file name will look like YEARMEANNone.IMO. If (a) a file called YEARMEAN.IMO is already existing within the selected directory a new line like

                       2022.500   4 47.2  64 26.6  21071  20997   1758  44062  48841 A XYZG

will be appended at the correct position. If (b) such YEARMEAN file is not yet existing, it will be newly created making use of information from the meta panel.

Please note: IAF contain data rounded to 0.1 nT. I usually prefer to create the IYVF input from my full resolution one-minute data product which I typically store as an CDF structure. Creating input lines for quiet days and disturbed days is currently only possible using backend methods.

Regarding BLV

This should be possible by using your analyzed basevalue data. Store this data after DI analysis, eventually already with the adopted baseline (using "ANALYSIS" -> "FIT"). When exporting such data you only will have three format options (BLV, PYCDF, and PYSTR). I typically keep a PYSTR (ascii) file which contains all underlying data from the DI analysis. Unfortunately, BLV is not yet working properly in the XMAGPY frontend - I get some permission denied error. I will dig into this and come back to you. (I typically use a quasi-automated backend script to create all my IM and IAGA dissimination files from my one-second definitive results).

mlnorthernswe commented 1 year ago

Thank you for the answer.

I wanted to export to IYFV with no full year data. It sounds unlogical but I use an software (imcdview: https://geomag.bgs.ac.uk/data_service/intermagnet/home.html) that use that file and I check data after each month we have cleaned the data (hence I don't have full year data).

Regarding BLV I did as you suggested in xmagpy. However the scalar data is not included in that file (it's marked with gaps (99999.00)) and hence delta F also is filled with gaps (888.00). How can I get scalar data included? It looks like this: 001 10481.50 31.86 52013.86 99999.00 888.00 c 002 10481.51 31.89 52013.86 99999.00 888.00 c 003 10481.52 31.90 52013.86 99999.00 888.00 c 004 10481.53 31.91 52013.87 99999.00 888.00 c 005 10481.54 31.92 52013.87 99999.00 888.00 c 006 10481.56 31.93 52013.87 99999.00 888.00 c

leonro commented 1 year ago

I did a number of changes to solve these issues. Firstly, I corrected the IYFV export scheme and, secondly, I included a number of options to XMagPy which were previously only accessible using backend methods. All updates will be included in version 1.1.3. Details below

IYVF:

BLV:

Changes are currently available within the develop branch and can be found here: 8e07a28dbf9873bbc3e66657d01d6775f50a822b bde5cdfe1aa85f9116f495c3c97bfee2a8f46055 d5453a5d0fa9fac8f50f4e57265d6c5cad52ee21

As soon as 1.1.3 is tagged, and provided that the issues are solved, I will close this one.

mlnorthernswe commented 1 year ago

It worked to install the develop branch with: pip3 install git+https://github.com/geomagpy/magpy.git@develop But xmagpy shows still version 1.1.2 in About. Is it correct? In venv I managed to install develop branch correctly so now I can test that branch.

leonro commented 1 year ago

No, develop version number should be something like1.1.3b00x. Good that you were able to install it using venv.

mlnorthernswe commented 1 year ago

I have tested a little. But I get the same result as before. I do like the following:

  1. I load the absolute measurements which are in MAGPYNEWABS-format from here: https://www2.irf.se/maggraphs/absolute_measurements/ (I choose 2022-12-29 to 2023-04-11). Vario/Scalar from here: https://www2.irf.se/maggraphs/vario_scalar/.
  2. I press "Analyze" (it should be good with feedback in xmagpy how far the analyze has reached (i.e what absolute measurement that is processed))
  3. I go the "Data" tab. As our Magnetometer measures XYZ I convert to XYZ by selecting xyz. I select columns X, Y, Z, H-base, D-base, Z-base and dF.
  4. I go back to "Analyzis" tab. Press "Fit". Choose the default settings and press "Apply".
  5. I go to "File" tab and export data by choosing "BLV".
  6. Choose Year: 2023. Adopted scalar F difference: default. Representative delta F source (one-minute): None. Apply.

The resulting file can be found here: https://www2.irf.se/maggraphs/absolute_measurements/KIR2023.blv

I also wonder about MAGPYNEWABS-format. In that format you can't present the "pillar difference" (baseline scalar F) value as it's added to the PPM values. In https://intermagnet.github.io/docs/Technical-Manual/technical_manual.pdf page 115 the IBF format is described and there that value should be presented but as that value is not included in MAGPYNEWABS I don't think that it's possible or am I wrong?

leonro commented 1 year ago

Just some quick clarification questions:

mlnorthernswe commented 1 year ago

Yes, our magnetometer is aligned along geographic coordinates XYZ (of course X to true north, and Y west and Z down).

I understand now what you mean with "small differences in scalar baselines". The scalar baseline is the pillar difference that we measure a couple of times each year. Between those measurements that baseline is you can say a constant, therefore the small differences. See page 115-116 in https://intermagnet.github.io/docs/Technical-Manual/technical_manual.pdf that defines IBFV2.00 format. See also page 17 about "CALCULATION OF THE DIFFERENCE BETWEEN F PILLAR AND ABSOLUTE PILLAR". As pillar diff is already included in MAGPYNEWABS format the scalar baseline will be 0 in IBFV2.00 or am I wrong? Therefore I miss scalar baseline in MAGPYNEWABS format.

This is our own BLV file if you want to compare: https://www.irf.se/observatory/mag/intermagnet_maglinux/cd/MAG2023/KIR/KIR2023.BLV But we are using a different spline method (monotonic spline (Steffen method: https://adsabs.harvard.edu/full/1990A%26A...239..443S) with the knots at the absolute measurements time points (bad absolute measurements filtered away)). I wanted that the baseline should contain the good absolute measurements as at those points the quality of data is best (dF->0 etc.), but at the same time the interpolation should be aware of trends from earlier and later absolute measurements which the Steffen method is suitable for.

No, not in place anyway, I will attend IAGA workshop. If there are online sessions I maybe can attend.

leonro commented 1 year ago

For now I have updated the README with detailed information on the DI-flux analysis and basevalue adoption technique as currently used by MagPy. In this section (https://github.com/geomagpy/magpy/tree/develop#2117-details-on-di-flux-analysis-and-calculation-of-basevalues) you will find basically all details and also a short section on scalar values and how they are incorporated into the result. In your case, the scalar values come from a separate pier. They are however also included into your individual DI data structure files. Thus , the analysis routine treats them as measurements at the same pier. Additionally, scalar data, corrected for pier diff, is provided from an external source. The routine calculates a pier difference between external data and the ones provided within the DI struct, which are identical and therefore pier diff is zero. As I understand so far for your data source, the DI data structures should not contain F values, as you don't have measurements at the DI-flux pier. You should only provide the raw data from your scalar source (vario/scalar button on DI panel) and provide the pier difference at the field dideltaF within the Analysis parameter window on the DI panel. This way, a correct BLV output will be obtained and delta F's as provided will be correctly stored. I hope the extension of the README helps. I also found an issue with baseline adoption if non-quasi absolute variations are used for DI analysis and corrected that. Furthermore I am working on a solution to also get XYZ BLV files in case of XYZ variation data (see also issue #123). Updates are available on develop branch and will be part of 1.1.3.

mlnorthernswe commented 1 year ago

Thanks for the thorough explanation. In the data in vario/scalar in DI panel I have already added pillar difference so dideltaF should be 0 there. I got however a rather different value in Y baseline compared to own calculations. D and I values are the same you can say for the absolute measurements (some decimals apart). I will test again if I get the same result and come back.

leonro commented 1 year ago

Just uploaded a new update into the development branch. The new version fully supports XYZ and HEZ variation data (and also basevalue outputs in XYZ). Further details are here https://github.com/geomagpy/magpy/issues/123#issuecomment-1545978716