Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Paras M. Solanki"'
Publikováno v:
Remote Sensing, Vol 15, Iss 7, p 1801 (2023)
Basalts from Mare Orientale are representative of lunar flood volcanism, which sheds light on the lunar farside’s thermal and volcanic past. We use Chandrayaan’s Moon Mineralogy Mapper data to examine the spectral and chemical makeup of the volca
Externí odkaz:
https://doaj.org/article/62084f26fb5546b8b6456c3701a9b28f
Publikováno v:
Journal of the Geological Society of India. 96:485-490
The stratigraphic sequence exposed in Wandhaya area comprises of marine clastic sediments of Mesozoic, which includes M-III and M-IV of Jumara Formation, Lower Member of Jhuran Formation and Upper Member of Bhuj Formation. Lithofacies erected from th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3fa37d701692362d197e2838eadaebe0
https://doi.org/10.1007/s12594-020-1586-x
https://doi.org/10.1007/s12594-020-1586-x
Autor:
Paras M Solanki, Shreekumari M Patel
Publikováno v:
Journal of the Indian Society of Remote Sensing. 48:1253-1263
In the present study, Landsat 8 Operational Land Imager multispectral data covering Gujarat's Kachchh district have been analyzed to map the Deccan Traps. The study area is covered by different lithological units from Middle Jurassic to Holocene rock
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::57389333ba546d7f86f734030c124a7c
https://doi.org/10.1007/s12524-020-01152-1
https://doi.org/10.1007/s12524-020-01152-1
Publikováno v:
Journal of Earth System Science. 130
Gassendi impact crater is located on the western side of the visible lunar hemisphere just north of Mare Humorum. It has a diameter of 110 km, and it is a Floor Fractured Crater (FFC) belonging to Class-3 type that exhibits a wide annular depression
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7a76cd24872a00f5c66019e1fea47e5d
https://doi.org/10.1007/s12040-021-01567-5
https://doi.org/10.1007/s12040-021-01567-5
Publikováno v:
Journal of Earth System Science. 129
The aim of the study was to observe two lunar impact craters of Copernican age, Ohm (18.4°N, 113.5°W) and Stevinus (32.5°S, 54.2°E) under microwave radar data of Miniature Radio Frequency (Mini-RF), an instrument onboard Lunar Reconnaissance Orbi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8850068cea9a1caae87d188911ef2ee5
https://doi.org/10.1007/s12040-020-1370-8
https://doi.org/10.1007/s12040-020-1370-8
Publikováno v:
Journal of the Geological Society of India. 90:396-404
On the basis of distinct lithologic features such as composition, grain size, bedding characteristics and sedimentary structures, six facies were identified in Callovian to Oxfordian rocks exposed southwest of Bhuj, Kachchh. They are interbedded calc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::68b21bb0b6dc7a711fcb37af746747b5
https://doi.org/10.1007/s12594-017-0734-4
https://doi.org/10.1007/s12594-017-0734-4
Publikováno v:
Journal of Palaeosciences. 65:67-84
Himmatnagar Sandstone (lower to middle Cretaceous) is exposed in between Sabarmati River in the west to Vantada in the east around Himmatnagar Town in north Gujarat, India. The sequence is divisible in two members: The lower member is 65 m thick, mos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6fe961f580ff305c50dd65410fe69346
https://doi.org/10.54991/jop.2016.300
https://doi.org/10.54991/jop.2016.300
Publikováno v:
Journal of Palaeosciences. 65:169-176
The state of Gujarat physiographically comprises three distinct zones–the Gujarat Mainland, the Saurashtra and the Kachchh. The sedimentary deposits of Himmatnagar Sandstone (23°36'00": 72°57'45") are mainly exposed in Gujarat Mainland. Palaeobot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0fdcc6bfe5ec79b951e0551f719c9ab9
https://doi.org/10.54991/jop.2016.308
https://doi.org/10.54991/jop.2016.308
Publikováno v:
Planetary and Space Science. 184:104856
The aim of this study is to analyze and compare morphological characters of three complex lunar impact craters- Crookes (10.3° S, 164.5° W), Ohm (18.4° N, 113.5° W) and Stevinus (32.5° S, 54.2° E), where Crookes and Ohm are located on the far s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9ea1c65e2c1a1ae758c47a9f3b9f65b8
https://doi.org/10.1016/j.pss.2020.104856
https://doi.org/10.1016/j.pss.2020.104856
Publikováno v:
Geosciences Research. 1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2b63f9fa040a335a81e6100d0745d00a
https://doi.org/10.22606/gr.2016.11003
https://doi.org/10.22606/gr.2016.11003