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Changes between Version 59 and Version 60 of RoboDIMM


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Timestamp:
Dec 7, 2010, 11:36:44 PM (16 years ago)
Author:
giebink
Comment:

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  • RoboDIMM

    v59 v60  
    474474=== __September 7, 2010__ ===
    475475
     476Locations 2,3, and 4.
    476477During the RoboDIMM observations I made last night at Reber Circle the wind was 3-6 m/s as measured at the DNSM and out of the SE. After struggling for nearly an hour trying to get the RoboDIMMs to track Vega, a star nearly as close to zenith as Altair, the star the DNSMwas tracking, I gave up and moved to Arcturus which was dropping to
    477478the west. The disparity in reported seeing values in the attached plot during this period appear to reflect the difference between the RoboDIMMs and the DNSM in the altitude of their respective target stars. Despite looking through quite a bit of atmosphere the RoboDIMMs seem to be fairly consistent.
     
    483484=== __September 10, 2010__ ===
    484485
     486Location 4 (labelled Location 2 on jpg)
     487
     488The attached plots shows data collected from the RoboDIMMs separated by a distance of about 40' on Reber Circle. Winds were close to 6 m/s early in the evening but dropped to just over 2 m/s by the end. High clouds necessitated moving the DIMMs to a number of different targets as well as repeatedly restarting the program and re-acquiring stars. The last hour was spent tracking a star quite low in the sky
     489
    485490 * [https://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/attachment/wiki/RoboDIMM/Reber-seeing-9.10.10.jpg Seeing Plot]
    486491
    487 The attached plots shows data collected from the RoboDIMMs separated by a distance of about 40' on Reber Circle. Winds were close to 6 m/s early in the evening but dropped to just over 2 m/s by the end. High clouds necessitated moving the DIMMs to a number of different targets as well as repeatedly restarting the program and re-acquiring stars. The last hour was spent tracking a star quite low in the sky
    488 
    489492=== __September 14, 2010__ ===
    490493
     49440 ft NW (labelled Location 2 on jpg)
     495
    491496Attached are last nights results. The winds were ~10m/s out of the E-SE during the evening. The static DIMM was sheltered from the wind somewhat by the PS2 containers. I believe this accounts for the differences between the DIMMs between 6:30 and 7. At that time I moved from a Arcturus which was fairly low to Rasalhague which was closer to zenith. Both DIMMs were affected by the wind but the one toward the center was buffeted more. Despite this, it appears that the measurements coincide well and it seems that we can conclude that seeing is relatively consistent across Reber Circle.
    492497
     
    495500=== __September 23, 2010__ ===
    496501
     502Airglow roof and Reber Circle center
     503
     504Plot only has short time segment where "fuzzball" event didn't occur
    497505
    498506 * [https://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/attachment/wiki/RoboDIMM/corrected-Reber-seeing-9.23.10.jpg Seeing Plot]
     
    500508=== __October 14, 2010__ ===
    501509
    502 In the attached plot the DNSM data is corrected to zenith and converted to FWHM, the RoboDIMM data is converted to FWHM, and the PS1 FWHM is directly out of the DB. Throughout the night the winds were < 5 m/s out of the NE. The large gap in the DNSM data is due to high clouds obscuring Altair. At 8 UT the DNSM moved to Diphda and resumed data collection. The high clouds moved across the RoboDIMM's path to Vega a few times requiring that the DIMMs be restarted. During the time period that RoboDIMM data was collected PS1 was pointed to the SE.
     510Airglow roof and Reber Circle center
     511
     512In the attached plot the DNSM data is corrected to zenith and converted to FWHM, the RoboDIMM data is converted to FWHM, and the PS1 FWHM is corrected for airmass. Throughout the night the winds were < 5 m/s out of the NE. The large gap in the DNSM data is due to high clouds obscuring Altair. At 8 UT the DNSM moved to Diphda and resumed data collection. The high clouds moved across the RoboDIMM's path to Vega a few times requiring that the DIMMs be restarted. During the time period that RoboDIMM data was collected PS1 was pointed to the SE.
    503513
    504514 * [https://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/attachment/wiki/RoboDIMM/corrected-Reber-seeing-10.14.10.jpg Seeing Plot]