https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Pierre_Kaufmann&feed=atom&action=historyPierre Kaufmann - Revision history2024-03-28T22:31:20ZRevision history for this page on the wikiMediaWiki 1.16.0https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Pierre_Kaufmann&diff=10783&oldid=prevSchriste at 19:00, 22 August 20182018-08-22T19:00:51Z<p></p>
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</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Pierre_Kaufmann&diff=9606&oldid=prevHhudson at 13:22, 14 March 20172017-03-14T13:22:47Z<p></p>
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</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Pierre_Kaufmann&diff=9550&oldid=prevHhudson at 13:59, 3 March 20172017-03-03T13:59:27Z<p></p>
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</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Pierre_Kaufmann&diff=9513&oldid=prevHhudson at 13:48, 24 February 20172017-02-24T13:48:01Z<p></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>flight of his Solar-T experiment - the first aimed at solar observations in the 1-10 THz band - as </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>flight of his Solar-T experiment - the first aimed at solar observations in the 1-10 THz band - as </div></td></tr>
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<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[https://antarcticsun.usap.gov/science/contenthandler.cfm?id=4270 GRIPS] <del class="diffchange diffchange-inline">experiment</del>.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[https://antarcticsun.usap.gov/science/contenthandler.cfm?id=4270 GRIPS] <ins class="diffchange diffchange-inline">balloon platform</ins>.</div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>His active interest in the analysis of <del class="diffchange diffchange-inline">these </del>novel data has now been cut short,</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>His active interest in the analysis of <ins class="diffchange diffchange-inline">the totally </ins>novel data <ins class="diffchange diffchange-inline">thus obtained </ins>has now been cut short,</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>much to our regret.</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>much to our regret.</div></td></tr>
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</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Pierre_Kaufmann&diff=9510&oldid=prevHhudson: draft of 2932017-02-24T10:50:35Z<p>draft of 293</p>
<p><b>New page</b></p><div>{{Infobox Nugget<br />
|name = Nugget<br />
|title = Pierre Kaufmann<br />
|number = 293<br />
|first_author = <br />
|second_author = <br />
|publish_date = 19 February 2017<br />
|next_nugget = Terrestrial gamma rays<br />
|previous_nugget = [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=RHESSI's_15th_Anniversary RHESSI's 15th Anniversary] <br />
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<br />
[[File:293f1.png|500px|thumb|center| <br />
Pierre Kaufmann, deceased February 17th 2017.<br />
]]<br />
<br />
RHESSI has lost a good friend and a great inspiration, as Pierre Kaufmann <br />
unexpectedly passed away February 17th 2017.<br />
His long research career emphasized technical innovation, observational novelty and exploration, especially in<br />
the radio domain at its shortest wavelengths, up into the infrared.,<br />
His dedication to these interests cleared the way for the first<br />
meaningful observation of solar magnetic activity across a <br />
surprisingly uncharted and broad swath of the electromagnetic spectrum, <br />
the submm/far-IR range 0.1-100 THz.<br />
His group's pioneering observation of a solar flare at 10 microns (which he<br />
thought of as 30 THz) fits in very nicely with RHESSI's imaging<br />
spectroscopy in the hard X-ray and gamma-ray domains (see Ref. [1]).<br />
this work has shown the way forward and also raised serious and interesting questions<br />
about the physical processes involved. <br />
<br />
It is worth noting that one of Pierre's last adventures was the successful<br />
flight of his Solar-T experiment - the first aimed at solar observations in the 1-10 THz band - as <br />
a piggyback experiment on the Berkeley/GSFC <br />
[https://antarcticsun.usap.gov/science/contenthandler.cfm?id=4270 GRIPS] experiment.<br />
His active interest in the analysis of these novel data has now been cut short,<br />
much to our regret.<br />
<br />
=== References ===<br />
<br />
[1] [http://adsabs.harvard.edu/abs/2015JGRA..120.4155K "Bright 30 THz impulsive solar bursts"]</div>Hhudson