Multi-Instrument Solar Flare Observations I: Solar Flare Finder

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From here, a user can search by:
From here, a user can search by:
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- GOES Class (B, C, M, X)
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* GOES Class (B, C, M, X)
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- Maximum Energy Detected by RHESSI
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* Maximum Energy Detected by RHESSI
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- Whether RHESSI observed most of the impulsive phase, or as long as it observed part of it
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* Whether RHESSI observed most of the impulsive phase, or as long as it observed part of it
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- Flare location (disc vs. limb) based on AIA locations
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* Flare location (disc vs. limb) based on AIA locations
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- Whether it was observed by other instruments such as EVE MEGS-A or MEGS-B, the 3 Hinode instruments or IRIS
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* Whether it was observed by other instruments such as EVE MEGS-A or MEGS-B, the 3 Hinode instruments or IRIS
==Search Method==
==Search Method==

Revision as of 15:32, 6 March 2017

Contents

Introduction

The solar physics community is fortunate to have access to a great deal of data from many solar observatories, both in space and on the ground. These instruments provide imaging, photometric, and spectroscopic data over a range of wavelengths, from radio waves through the optical and EUV to X-rays and gamma-rays. Often the greatest advances in our understanding of solar flares come through various combinations of these datasets. However, unless one is an instrument planner or someone who monitors daily solar activity, It is difficult to keep track of which flares have been observed by which instruments. The RHESSI-funded Max Millennium Program for Solar Flare Research (Ref. 1) and others have aimed to optimise the scientific return on our data by coordinating ground and space based instrumentation to observe a flaring active region simultaneously. However, this can be difficult due to factors such as coordinating across multiple time zones, planning schedules being uploaded days in advance, ground-based seeing conditions, competing scientific priorities, and so on. Indeed, shortly after RHESSI first light, joint multi-wavelength observations of solar flares were strongly encouraged. To this end an IDL widget has been developed to retrospectively search metadata from the archival databases of RHESSI, SDO/EVE (MEGS-A and MEGS-B), Hinode (EIS, SOT and XRT) and IRIS for flaring events jointly observed by multiple instruments. Simply type IDL> solar_flare_finder at the command line to bring up this window:

Figure 1: Screenshot of the SOLAR_FLARE_FINDER widget in SSWIDL.

From here, a user can search by:

Search Method

The SSWIDL widget searches a pre-generated lookup table to instantly return a list of flares corresponding to the users criteria. The construction of the table begins with the SSW Latest Events list, which is accessible via the HEK. This list is based on the familiar NOAA GOES event list except it contains the location information of each flare based on SDO/AIA 131A difference images. This is required to compare with limited FOV instruments.

Biographical Note

Ryan Milligan is currently an Ernest Rutherford Fellow at the University of Glasgow.

References

[1] "Performance of Major Flare Watches from the Max Millennium Program (2001 - 2010)"

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