2024-09-24T22:22:04.000Z http://sot.lmsal.com Mr. Sam Freeland Lockheed Martin Solar and Astrophysics Laboratory (LMSAL) http://www.lmsal.com Lockheed Martin Advanced Tech Center, 3251 Hanover Rd, O/ADBS, B/252, Palo Alto, CA 94304 null null HINODE SOTSP Hosoi Brooks Cruz (RCO) 313 HOP 313 @ Disk Center disk center JET JET N/A 17 20160613_065955 246 269 281 17 76 313 2 1 1 2 0 21 2028 156 0.9968051118210862 0.184 7.318 49.452 121.728 2016-06-13T06:59:55.000Z 2016-06-13T07:09:46.000Z 0.184 7.318 A Search Chromospheric Manifestation of Ubiquitous Photospheric Jets Fast Map, 50"x122", Q75 1-side CCD, Repeat 1 request to SOT Request initially one-hour time sequences using the SP ?very fast mode?observational mode. Observations should be taken in dual-beam mode (acquisition of both sides of the SP CCD). An SP very fast map of 9? width (30 digitized steps of 0.297? each) requires 72 seconds. The effective pixel size is twice that possible with the SP, but analysis of prior observations of these photospheric events indicates that this resolution is sufficient to identify them and to carry out detailed analysis. Both sides of the CCD will be digitized in order to enhance the signal-to-noise ratio, and to minimize effects of polarization crosstalk from residual image motion and solar evolution. The data acquisition will be limited to 768 pixels along the SP slit (384 digitized pixels, or 123?) to match the full length of the IRIS slit (120?). Based upon prior observations of the photospheric jets, we expect to capture of the order of 20 events in 3-4 hours of observation. In order to build up significant statistics, we would like to plan for the initial observing program to acquire about 20 orbits of co-aligned data, which should yield about 200 separate events. This initial data will be subjected to analysis before proceeding with additional observations.;;request to SOT Request initially one-hour time sequences using the SP ?very fast mode?observational mode. Observations should be taken in dual-beam mode (acquisition of both sides of the SP CCD). An SP very fast map of 9? width (30 digitized steps of 0.297? each) requires 72 seconds. The effective pixel size is twice that possible with the SP, but analysis of prior observations of these photospheric events indicates that this resolution is sufficient to identify them and to carry out detailed analysis. Both sides of the CCD will be digitized in order to enhance the signal-to-noise ratio, and to minimize effects of polarization crosstalk from residual image motion and solar evolution. The data acquisition will be limited to 768 pixels along the SP slit (384 digitized pixels, or 123?) to match the full length of the IRIS slit (120?). Based upon prior observations of the photospheric jets, we expect to capture of the order of 20 events in 3-4 hours of observation. In order to build up significant statistics, we would like to plan for the initial observing program to acquire about 20 orbits of co-aligned data, which should yield about 200 separate events. This initial data will be subjected to analysis before proceeding with additional observations. ivo://sot.lmsal.com/VOEvent#2016-06-13T06:59:30Z