<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
 <record>
  <leader>     caa a22        4500</leader>
  <controlfield tag="001">445346175</controlfield>
  <controlfield tag="003">CHVBK</controlfield>
  <controlfield tag="005">20180317142829.0</controlfield>
  <controlfield tag="007">cr unu---uuuuu</controlfield>
  <controlfield tag="008">170323e20110601xx      s     000 0 eng  </controlfield>
  <datafield tag="024" ind1="7" ind2="0">
   <subfield code="a">10.1007/s11207-011-9777-7</subfield>
   <subfield code="2">doi</subfield>
  </datafield>
  <datafield tag="035" ind1=" " ind2=" ">
   <subfield code="a">(NATIONALLICENCE)springer-10.1007/s11207-011-9777-7</subfield>
  </datafield>
  <datafield tag="245" ind1="0" ind2="4">
   <subfield code="a">The RHESSI Microflare Height Distribution</subfield>
   <subfield code="h">[Elektronische Daten]</subfield>
   <subfield code="c">[S. Christe, S. Krucker, P. Saint-Hilaire]</subfield>
  </datafield>
  <datafield tag="520" ind1="3" ind2=" ">
   <subfield code="a">We present the first in-depth statistical survey of flare source heights observed by RHESSI. Flares were found using a flare-finding algorithm designed to search the 6 - 10keV count-rate when RHESSI's full sensitivity was available in order to find the smallest events (Christe etal. in Astrophys.J. 677, 1385, 2008). Between March 2002 and March 2007, a total of 25 006 events were found. Source locations were determined in the 4 - 10keV, 10 - 15keV, and 15 - 30keV energy ranges for each event. In order to extract the height distribution from the observed projected source positions, a forward-fit model was developed with an assumed source height distribution where height is measured from the photosphere. We find that the best flare height distribution is given by g(h)∝exp (−h/λ) where λ=6.1±0.3Mm is the scale height. A power-law height distribution with a negative power-law index, γ=3.1±0.1 is also consistent with the data. Interpreted as thermal loop-top sources, these heights are compared to loops generated by a potential-field model (PFSS). The measured flare heights distribution are found to be much steeper than the potential-field loop height distribution, which may be a signature of the flare energization process.</subfield>
  </datafield>
  <datafield tag="540" ind1=" " ind2=" ">
   <subfield code="a">Springer Science+Business Media B.V. (outside the USA), 2011</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Christe</subfield>
   <subfield code="D">S.</subfield>
   <subfield code="u">NASA Goddard Space Flight Center, 20771-0001, Greenbelt, MD, USA</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Krucker</subfield>
   <subfield code="D">S.</subfield>
   <subfield code="u">Space Sciences Laboratory, University of California at Berkeley, 94720-7450, Berkeley, CA, USA</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Saint-Hilaire</subfield>
   <subfield code="D">P.</subfield>
   <subfield code="u">Space Sciences Laboratory, University of California at Berkeley, 94720-7450, Berkeley, CA, USA</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="773" ind1="0" ind2=" ">
   <subfield code="t">Solar Physics</subfield>
   <subfield code="d">Springer Netherlands</subfield>
   <subfield code="g">270/2(2011-06-01), 493-502</subfield>
   <subfield code="x">0038-0938</subfield>
   <subfield code="q">270:2&lt;493</subfield>
   <subfield code="1">2011</subfield>
   <subfield code="2">270</subfield>
   <subfield code="o">11207</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="0">
   <subfield code="u">https://doi.org/10.1007/s11207-011-9777-7</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="908" ind1=" " ind2=" ">
   <subfield code="D">1</subfield>
   <subfield code="a">research-article</subfield>
   <subfield code="2">jats</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">856</subfield>
   <subfield code="E">40</subfield>
   <subfield code="u">https://doi.org/10.1007/s11207-011-9777-7</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Christe</subfield>
   <subfield code="D">S.</subfield>
   <subfield code="u">NASA Goddard Space Flight Center, 20771-0001, Greenbelt, MD, USA</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Krucker</subfield>
   <subfield code="D">S.</subfield>
   <subfield code="u">Space Sciences Laboratory, University of California at Berkeley, 94720-7450, Berkeley, CA, USA</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Saint-Hilaire</subfield>
   <subfield code="D">P.</subfield>
   <subfield code="u">Space Sciences Laboratory, University of California at Berkeley, 94720-7450, Berkeley, CA, USA</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">773</subfield>
   <subfield code="E">0-</subfield>
   <subfield code="t">Solar Physics</subfield>
   <subfield code="d">Springer Netherlands</subfield>
   <subfield code="g">270/2(2011-06-01), 493-502</subfield>
   <subfield code="x">0038-0938</subfield>
   <subfield code="q">270:2&lt;493</subfield>
   <subfield code="1">2011</subfield>
   <subfield code="2">270</subfield>
   <subfield code="o">11207</subfield>
  </datafield>
  <datafield tag="900" ind1=" " ind2="7">
   <subfield code="a">Metadata rights reserved</subfield>
   <subfield code="b">Springer special CC-BY-NC licence</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="898" ind1=" " ind2=" ">
   <subfield code="a">BK010053</subfield>
   <subfield code="b">XK010053</subfield>
   <subfield code="c">XK010000</subfield>
  </datafield>
  <datafield tag="949" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="F">NATIONALLICENCE</subfield>
   <subfield code="b">NL-springer</subfield>
  </datafield>
 </record>
</collection>
