[Loops] summaries on nanoflare debates in "coronalloopworkshops"
Petrus Martens
pmartens at cfa.harvard.edu
Fri Mar 6 15:07:21 MST 2009
Leon,
Dense as a brick... I am not replying to Markus' input anymore.
You're right about our Italian friends though. Once I am done with
tons of SDO-SC related organizing and resubmitting my loop paper,
there is a whole sequence of papers with Trae on coronal loops and
flares in queue.
Cheers,
Piet
Leon Golub wrote:
> OK, I have to jump in, since there seems to be some confusion about
> this. Yes, the increase in coronal density comes up from the
> chromosphere. This has been known for decades and has been well-modeled,
> especially by the Palermo group. But it is entirely possible for the
> energy to be deposited in the corona, then travel down (relying on the
> ambient density) to be deposited and cause evaporation. The pattern of
> brightness variations that you see does, in fact, change depending on
> where in the loop the energy is deposited, and can be used to determine
> where it happened. By seeing how the loop brightens, you can tell where
> the energy deposition took place. See:
>
>> A Brightening Coronal Loop Observed by TRACE. II. Loop Modeling and Constraints on Heating
>> Reale, F.; Peres, G.; Serio, S.; Betta, R. M.; DeLuca, E. E.; Golub, L.
>> Astrophysical Journal, Volume 535, Issue 1, pp. 423-437, 05/2000.
>
> Leon
>
>
> Markus J. Aschwanden wrote:
>> On Mar 6, 2009, at 8:44 AM, Klimchuk, James A. (GSFC-6710) wrote:
>>
>>> By the way, I do NOT believe that observations necessarily point to low
>>> altitude heating. My view is that observations are consistent with both
>>> low altitude and high altitude heating. Perhaps this should be a topic
>>> for Loops IV.
>>>
>>> Jim
>> There is no way around to heat up first chromospheric material to fill
>> coronal
>> loops to produce the enhanced soft X-ray and EUV emission we see from
>> coronal loops (like in flares). Any heating mechanism that heats directly
>> in the corona, does not increase the local density, so we would not see
>> any loops.
>>
>> Markus
>>
>>
>>
>> ____________________________________________
>> Dr. Markus J. Aschwanden
>> Solar & Astrophysics Laboratory
>> Lockheed Martin Advanced Techology Center
>> Org. ADBS, Bldg. 252
>> 3251 Hanover St., Palo Alto, CA 94304, USA
>> Phone: 650-424-4001, FAX: 650-424-3994
>> URL: http://www.lmsal.com/~aschwand/
>> e-mail: aschwanden at lmsal.com <mailto:aschwanden at lmsal.com>
>> _______________________________________
>> ____________________________________
>>
>>
>>
>>
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