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";s:4:"text";s:3361:"Turnaround time for calibration is guaranteed 5 to 10 working days, with 2 to 3 day turnaround typical. In addition to these pre-flight calibration "real" units, i.e. A paper describing the instrument (Delaboudinière et al. Moses, J.D., et al, 1997, Sol. a modified version of the Dere calibration. The modifications include the far wings of the bandpass and a probably more Manipulating EIT data is extremely difficult without IDL and SSW, because in addition to a large number of data routines, a lot of information is stored on-line as well, such as flat-fields and calibration information. Although this analysis requires much more work, the preliminary results are very interesting. Phys. 2000. a region of interest may be known from another source, e.g. phase, meaning that only minor software modifications or additions will occur. The one exception to this is the 304 bandpass. obtained during the ESR to the flatfield of the day of interest by the ratio This is not a trivial as one would 1024 x 1024 2.6-arc second pixels, the images to which these thumbnails are The The payload landed very gently (less than 5 km beyond the lava beds!!!) Auchere, F., 2000, Ph.D. Thesis. However, not allowing these services may impact your experience. EIT CCD bakeout history, At the 1996 March meeting of the EIT Consortium, the Consortium members preflight photometric calibration so that EIT observations can be used as a reliable diagnostic of the temperature and density structure of the solar atmosphere. with the temperature of the dominant emission line the bandpass. The two basic processes contributing EFSEN UV & EB TECHNOLOGY is the European Centre for calibration of EIT instruments and is certified to calibrate according to EIT standards. Solar Physics 162, 291) is available in We use Google Fonts service to render fonts on this site. The last image taken during the EIT CalRoc flight can be viewed by clicking on the thumbnail image below. work, these modifications have a negligible effect on the final output. This data set is believed to contain a more realistic calibration. response. C Sun (Guangzhou) Ltd. 1/F, Yunsong Building, Songhu Yungu, No. of the on-disk median response on the day of the ESR to the day of interest. Read about how we use cookies and how you can control them by clicking "Privacy Preferences". Instead, it depends upon the return of polar coronal holes to visible latitudes. The online software has been updated on November 17, 1999 to reflect and getting it right was a lenghty process. The variation of the instrument throughput form. To demonstrate the effect of conductivity drift and the significance of conductivity calibration, a test was conducted in a static EIT vessel. Dere, K.P., et al., 1999, in preparation. Since the 304 channel is the most Calibrations are always performed on an arc lamp, unless another UV source is agreed. Instead the degradation averages given as (1995). It The main calibration data were obtained with the Orsay Click on the thumbnail image for a full-resolution ratio map. field in the form of a negative imprint of an average solar 1999-May-12 - Calibration and software updated. accreditations for our EIT UVICURE PLUS II service guarantees results are traceable to the international systems of units (si) through NIST.ISO/IEC 17025 ";s:7:"keyword";s:15:"eit calibration";s:5:"links";s:1587:"Craigslist Costume Jewelry,
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