Caius' Notes - Revision history

Xingyao: /* EOVSA flare spectrograms */

2024-08-05T13:19:27Z

EOVSA flare spectrograms

← Older revision		Revision as of 13:19, 5 August 2024
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	The tpk (Time of the peak) determines the name of the resulting files (.png and .fits), and also determines the flare_id.		The tpk (Time of the peak) determines the name of the resulting files (.png and .fits), and also determines the flare_id.

	It's better to keep the formate of tpk as tpk='yyyy-mm-dd hh:mm:00' and add the flare time on wiki in the format of "hh:mm":		It's better to keep the formate of tpk as tpk='yyyy-mm-dd hh:mm:00' and add the flare time on wiki in the format of "hh:mm":

2024-08-05T13:19:07Z

EOVSA flare spectrograms

← Older revision		Revision as of 13:19, 5 August 2024
Line 82:		Line 82:

	The tpk (Time of the peak) determines the name of the resulting files (.png and .fits), and also determines the flare_id.		The tpk (Time of the peak) determines the name of the resulting files (.png and .fits), and also determines the flare_id.
	It's better to keep the formate of tpk as tpk='yyyy-mm-dd hh:mm:00':		It's better to keep the formate of tpk as tpk='yyyy-mm-dd hh:mm:00' and add the flare time on wiki in the format of "hh:mm":

	<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>		<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>

2024-07-26T18:21:55Z

EOVSA flare spectrograms

← Older revision		Revision as of 18:21, 26 July 2024
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	Use the figure above to choose the background interval (bgidx), the maximum intensity and the frequencies.		Use the figure above to choose the background interval (bgidx), the maximum intensity and the frequencies.
	The tpk (Time of the peak) determines the name of the resulting files (.png and .fits), and it's better to keep the formate of tpk as tpk='yyyy-mm-dd hh:mm:00':
			The tpk (Time of the peak) determines the name of the resulting files (.png and .fits), and also determines the flare_id.
			It's better to keep the formate of tpk as tpk='yyyy-mm-dd hh:mm:00':

	<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>		<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>

2024-07-26T18:20:18Z

EOVSA flare spectrograms

← Older revision		Revision as of 18:20, 26 July 2024
Line 80:		Line 80:

	Use the figure above to choose the background interval (bgidx), the maximum intensity and the frequencies.		Use the figure above to choose the background interval (bgidx), the maximum intensity and the frequencies.
	The tpk (Time of the peak) determines the name of the resulting files (.png and .fits):		The tpk (Time of the peak) determines the name of the resulting files (.png and .fits), and it's better to keep the formate of tpk as tpk='yyyy-mm-dd hh:mm:00':

	<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>		<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>

2024-07-26T18:17:46Z

EOVSA flare spectrograms

← Older revision		Revision as of 18:17, 26 July 2024
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	<pre style="font-family:courier">import glob		<pre style="font-family:courier">import glob
	files = sorted(glob.glob('IDB*')) </pre>		files = sorted(glob.glob('IDB*')) </pre>


	When all the antennas were fine, enter the following:		When all the antennas were fine, enter the following:

2024-07-26T18:17:21Z

EOVSA flare spectrograms

← Older revision		Revision as of 18:17, 26 July 2024
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	Or all the IDB files can be read as:		Or all the IDB files can be read as:

	<pre style="font-family:courier">files = sorted(glob.glob('IDB*')) </pre>		<pre style="font-family:courier">import glob
			files = sorted(glob.glob('IDB*')) </pre>

2024-07-26T18:16:21Z

EOVSA flare spectrograms

← Older revision		Revision as of 18:16, 26 July 2024
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	<pre style="font-family:courier">files = ['IDB20240507162024','IDB20240507163024'] </pre>		<pre style="font-family:courier">files = ['IDB20240507162024','IDB20240507163024'] </pre>

			Or all the IDB files can be read as:

			<pre style="font-family:courier">files = sorted(glob.glob('IDB*')) </pre>


	When all the antennas were fine, enter the following:		When all the antennas were fine, enter the following:

2024-06-04T17:21:21Z

← Older revision		Revision as of 17:21, 4 June 2024
Line 85:		Line 85:
	In this example, the output files are eovsa.spec.flare_id_20240507163000.fits and eovsa.spec.flare_id_20240507163000.fits.		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:		At the end, copy the .fits file to /common/webplots/events/2024:

	<pre style="font-family:courier"> cp eovsa.spec.flare_id_20240507163000.fits /common/webplots/events/2024 </pre>		<pre style="font-family:courier"> cp eovsa.spec.flare_id_20240507163000.fits /common/webplots/events/2024 </pre>

2024-06-04T17:04:40Z

← Older revision		Revision as of 17:04, 4 June 2024
Line 75:		Line 75:

	Use the figure above to choose the background interval (bgidx), the maximum intensity and the frequencies.		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):		The tpk (Time of the peak) determines 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>		<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>

2024-05-30T17:09:12Z

EOVSA flare spectrograms

← Older revision		Revision as of 17:09, 30 May 2024
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	The tpk is defined as the name of the resulting files (.png and .fits):		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,~~220~~],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>		<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\|]]		[[File:eovsa.spec.flare_id_20240507163000.png\|none\|thumb\|center\|500px\|]]