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High-latitude crochet (Solar flare effect) as a trigger of pseud-substorm onset
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<p>Solar flares are known to enhance the ionospheric electron density and thus influence the electric currents in the D- and E-region. &#160;The geomagnetic disturbance caused by this current system is called a "crochet" or "SFE (solar flare effect)". &#160;Crochets are observed at dayside low-latitudes with a peak near the subsolar region ("subsolar crochet"), in the nightside high-latitude auroral region with a peak where the geomagnetic disturbance pre-exists during solar illumination ("auroral crochet"), and in the cusp ("cusp crochet"). &#160;In addition, we recently found a new type of crochet on the dayside ionospheric current at high latitudes (European sector 70-75 geographic latitude/67-72 geomagnetic latitude) independent from the other crochets. &#160;The new crochet is much more intense and longer in duration than the subsolar crochet and is detected even in AU index for about half the >X2 flares despite the unfavorable latitudinal coverage of the AE stations (~65 geomagnetic latitude) to detect this new crochet (Yamauchi et al., 2020). &#160;</p><p>The signature is sometime s seen in AL, causing the crochet signature convoluting with substorms. &#160;From a theoretical viewpoint, X-flares that enhances the ionospheric conductivity may influence the substorm activity, like the auroral crochet. &#160;To understand the substorm-crochet relation in the dayside, we examined SuperMAG data for cases when the onset of the substorm-like AL (SML) behavior coincides with the crochet. &#160;We commonly found a large counter-clockwise &#8710;B vortex centered at 13-15 LT, causing an AU peak during late afternoon and an AL peak near noon at higher latitudes than the high-latitude crochet. &#160;In addition, we could recognize a clockwise &#8710;B vortex in the prenoon sector, causing another poleward &#8710;B, but this signature is not as clear as the afternoon vortex. &#160;With such strong vortex features, it becomes similar to substorms except for its local time. &#160;In some cases, the vortex expends to the nightside sector, where and when nightside onset starts, suggesting triggering of onset. &#160;Thus, the crochet may behave like pseudo-onset at different latitude than midnight substorms, and may even trigger substorm onset.</p>
Title: High-latitude crochet (Solar flare effect) as a trigger of pseud-substorm onset
Description:
<p>Solar flares are known to enhance the ionospheric electron density and thus influence the electric currents in the D- and E-region.
&#160;The geomagnetic disturbance caused by this current system is called a "crochet" or "SFE (solar flare effect)".
&#160;Crochets are observed at dayside low-latitudes with a peak near the subsolar region ("subsolar crochet"), in the nightside high-latitude auroral region with a peak where the geomagnetic disturbance pre-exists during solar illumination ("auroral crochet"), and in the cusp ("cusp crochet").
&#160;In addition, we recently found a new type of crochet on the dayside ionospheric current at high latitudes (European sector 70-75 geographic latitude/67-72 geomagnetic latitude) independent from the other crochets.
&#160;The new crochet is much more intense and longer in duration than the subsolar crochet and is detected even in AU index for about half the >X2 flares despite the unfavorable latitudinal coverage of the AE stations (~65 geomagnetic latitude) to detect this new crochet (Yamauchi et al.
, 2020).
&#160;</p><p>The signature is sometime s seen in AL, causing the crochet signature convoluting with substorms.
&#160;From a theoretical viewpoint, X-flares that enhances the ionospheric conductivity may influence the substorm activity, like the auroral crochet.
&#160;To understand the substorm-crochet relation in the dayside, we examined SuperMAG data for cases when the onset of the substorm-like AL (SML) behavior coincides with the crochet.
&#160;We commonly found a large counter-clockwise &#8710;B vortex centered at 13-15 LT, causing an AU peak during late afternoon and an AL peak near noon at higher latitudes than the high-latitude crochet.
&#160;In addition, we could recognize a clockwise &#8710;B vortex in the prenoon sector, causing another poleward &#8710;B, but this signature is not as clear as the afternoon vortex.
&#160;With such strong vortex features, it becomes similar to substorms except for its local time.
&#160;In some cases, the vortex expends to the nightside sector, where and when nightside onset starts, suggesting triggering of onset.
&#160;Thus, the crochet may behave like pseudo-onset at different latitude than midnight substorms, and may even trigger substorm onset.
</p>.
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