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The longest total solar eclipse during the 21st century occurred in South and East Asia on July 22, 2009. Ionospheric response to this rare total solar eclipse which was observed right from the time of sunrise in the Indian zone, has been studied in terms of the total electron content (TEC) obtained from three global positioning system (GPS) receivers located at Udaipur, Hyderabad and Bengaluru, and electron density obtained using space based GPS-Radio Occultation technique. The study reveals significant reductions in the electron density and TEC that persisted up to 2 h past the last contact even during early morning eclipse. These observations imply that during the early morning eclipse, the production and loss of ionization dominate over the plasma transport processes. 相似文献
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Ajay Dashora B. Sreenivas Bharat Lohani Javed N. Malik Afroz Ahmad Shah 《Journal of the Indian Society of Remote Sensing》2006,34(2):153-160
Use of high-resolution and historic CORONA satellite photographs for mapping and other purposes requires Ground Control Points
(GCPs), as ephemeris data and image parameters are not available. However, the alterations in landscape in last 34 years (i.e., since the acquisition of these photographs) prevent identification and collection of large number of GCPs in the field.
This paper presents a methodology for collection of GCPs for CORONA photographs. The advantages and limitations of the methodology
are discussed. For a study site, situated in Siwaliks and Lower Himalayas, the GCPs were identified in CORONA photographs
and their WGS84 coordinates were estimated through a process of datum transformation and georeferencing. Estimated GCP coordinates
from the topo sheets and 2D and 3D views of photographs, helped in identifying the GCP locations in field, which were observed
using DGPS. Investigations were carried out to relate Differential Global Positioning System (DGPS) accuracy with base line
length and time of observation. Abase line of 350 km and half an hour observation were found appropriate to yield accuracy
in GCP collection by DGPS method, which conforms to CORONA resolution of 3 m. 相似文献
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We propose a criterion for extending the parameter search method (Krishnakumar and Venkatakrishnan, 1997) of estimating the point spread function to solar data. In the parameter search method, the number of pixels with negative intensity values in the restored object is used as an estimator for determining the unknown parameters of the point spread function. As a solar image has a high background, the restored object does not contain negative values, thereby making the method unsuitable for solar data. We propose to use the intrinsic contrast of solar features as a criterion for identifying the unknown parameter. We validate our method through simulations. This method can not be used for image restoration but can be used for monitoring daytime seeing. 相似文献
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Praveen Galav N. Dashora S. Sharma R. Pandey 《Journal of Atmospheric and Solar》2010,72(17):1309-1317
We present the mean diurnal, seasonal and annual variations in TEC during the lowest solar activity phase from low latitude Indian zone recorded at Udaipur (Geog. Lat. 24.6°N, Geog. Long.73.7°E, Geomag. Lat. 15.6°N) using a GPS receiver. Seasonal variations in daytime TEC show a semiannual periodicity, with a minimum in winter. Results of seasonal variations have been compared with that of the IRI-2007 model. Model calculations reveal significant seasonal as well as longitudinal differences in TEC. Seasonal variations in the nighttime TEC reveal an annual periodicity. Near the crest of the EIA, TEC shows a very good correlation with the solar flux. The results also point to weakening of the anomaly crest as well as its spatial and temporal contraction with declining solar activity. 相似文献
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