Caius' Notes: Difference between revisions
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== EOVSA | == EOVSA flare spectrograms == | ||
=== Checking the possible EOVSA === | |||
Verify the possible flares on the daily EOVSA Solar Dynamic Spectrogram, for example: | |||
http://ovsa.njit.edu/browser/?suntoday_date=2024-05-07 | |||
[[File:Daily_spec_20240507.png|none|thumb|center|500px|]] | |||
In this example, we are going to analyze the M8.2 flare that happened after 16:00 UT. | |||
For a better flare time precision, a Dynamic spectrogram with short time range at: | |||
http://ovsa.njit.edu/flaremon/ | |||
[[File:XSP20240507153014.png|none|thumb|center|500px|]] | |||
Since 2024-May-05, the Real Time Flare detection figure and its list are also available: | |||
http://ovsa.njit.edu/flaremon/FLM20240507.png | |||
http://ovsa.njit.edu/flaremon/flarelist/flarelist_2024-05-07.txt | |||
[[File:FLM20240507.png|none|thumb|center|500px|]] | |||
=== Using Python 3.8 === | |||
Login into pipeline machine as user: | |||
<pre style="font-family:courier">ssh -X user@pipeline </pre> | |||
To verify the antennas that were working, check the observing log http://ovsa.njit.edu/wiki/index.php/2024_May, | |||
or consult the TPCAL log file, e.g. more /dppdata1/TPCAL/LOG/TPCyyyymmdd.log | |||
Create the flare directory at /data1/dgary/solar/, e.g: | |||
<pre style="font-family:courier">mkdir 20240507_M8flare | |||
cd 20240507_M8flare</pre> | |||
Load the Python 3.8 environment: | |||
<pre style="font-family:courier">bash | |||
loadpyenv3.8 | |||
ipython --pylab</pre> | |||
In Python, enter the following: | |||
<pre style="font-family:courier">from eovsapy import flare_spec as fs | |||
from eovsapy.util import Time </pre> | |||
To download the IDB directories form the SQL cloud, enter the flare interval as: | |||
<pre style="font-family:courier">files = fs.calIDB(Time(['2024-05-07 16:20','2024-05-07 16:35'])) </pre> | |||
If the IDB already exist, they can be read as: | |||
<pre style="font-family:courier">files = ['IDB20240507162024','IDB20240507163024'] </pre> | |||
When all the antennas were fine, enter the following: | |||
<pre style="font-family:courier">out, spec = fs.inspect(files) </pre> | |||
But, if one or more antennas weren't working, enter the list of the good ones as: | |||
<pre style="font-family:courier"> out, spec = fs.inspect(files, ant_str='ant1-6 ant8-9 ant11-13') </pre> | |||
[[File:Out_spec.png|none|thumb|center|500px|]] | |||
To better see the flare, you can change the spec vmax as: | |||
<pre style="font-family:courier"> imshow(spec,vmax=30,vmin=-1) </pre> | |||
[[File:Out_spec2.png|none|thumb|center|500px|]] | |||
Use the figure above to choose the background interval (bgidx), the maximum intensity and the frequencies. | |||
The tpk is defined as the name of the resulting files (.png and .fits): | |||
<pre style="font-family:courier"> f, ax0, ax1 = fs.make_plot(out,bgidx=[200,210],vmin=0.1, vmax=110, lcfreqs=[120,190,270,350],ant_str='ant1-6 ant8-9 ant11-13', tpk='2024-05-07 16:30:00') </pre> | |||
[[File:eovsa.spec.flare_id_20240507163000.png|none|thumb|center|500px|]] | |||
A second background interval can be defined right after the first one, e.g., bg2idx=[1000,1010] | |||
In this example, the output files are eovsa.spec.flare_id_20240507163000.fits and eovsa.spec.flare_id_20240507163000.fits. | |||
At the end, copy .fits file to /common/webplots/events/2024: | |||
<pre style="font-family:courier"> cp eovsa.spec.flare_id_20240507163000.fits /common/webplots/events/2024 </pre> | |||
and include the flare in the wiki Flare List: | |||
http://ovsa.njit.edu/wiki/index.php/2024 | |||
The flare position have been copied from the https://solarmonitor.org/ |
Latest revision as of 17:09, 30 May 2024
EOVSA flare spectrograms
Checking the possible EOVSA
Verify the possible flares on the daily EOVSA Solar Dynamic Spectrogram, for example:
http://ovsa.njit.edu/browser/?suntoday_date=2024-05-07
In this example, we are going to analyze the M8.2 flare that happened after 16:00 UT.
For a better flare time precision, a Dynamic spectrogram with short time range at:
http://ovsa.njit.edu/flaremon/
Since 2024-May-05, the Real Time Flare detection figure and its list are also available:
http://ovsa.njit.edu/flaremon/FLM20240507.png http://ovsa.njit.edu/flaremon/flarelist/flarelist_2024-05-07.txt
Using Python 3.8
Login into pipeline machine as user:
ssh -X user@pipeline
To verify the antennas that were working, check the observing log http://ovsa.njit.edu/wiki/index.php/2024_May,
or consult the TPCAL log file, e.g. more /dppdata1/TPCAL/LOG/TPCyyyymmdd.log
Create the flare directory at /data1/dgary/solar/, e.g:
mkdir 20240507_M8flare cd 20240507_M8flare
Load the Python 3.8 environment:
bash loadpyenv3.8 ipython --pylab
In Python, enter the following:
from eovsapy import flare_spec as fs from eovsapy.util import Time
To download the IDB directories form the SQL cloud, enter the flare interval as:
files = fs.calIDB(Time(['2024-05-07 16:20','2024-05-07 16:35']))
If the IDB already exist, they can be read as:
files = ['IDB20240507162024','IDB20240507163024']
When all the antennas were fine, enter the following:
out, spec = fs.inspect(files)
But, if one or more antennas weren't working, enter the list of the good ones as:
out, spec = fs.inspect(files, ant_str='ant1-6 ant8-9 ant11-13')
To better see the flare, you can change the spec vmax as:
imshow(spec,vmax=30,vmin=-1)
Use the figure above to choose the background interval (bgidx), the maximum intensity and the frequencies. The tpk is defined as the name of the resulting files (.png and .fits):
f, ax0, ax1 = fs.make_plot(out,bgidx=[200,210],vmin=0.1, vmax=110, lcfreqs=[120,190,270,350],ant_str='ant1-6 ant8-9 ant11-13', tpk='2024-05-07 16:30:00')
A second background interval can be defined right after the first one, e.g., bg2idx=[1000,1010]
In this example, the output files are eovsa.spec.flare_id_20240507163000.fits and eovsa.spec.flare_id_20240507163000.fits.
At the end, copy .fits file to /common/webplots/events/2024:
cp eovsa.spec.flare_id_20240507163000.fits /common/webplots/events/2024
and include the flare in the wiki Flare List:
http://ovsa.njit.edu/wiki/index.php/2024
The flare position have been copied from the https://solarmonitor.org/