Zobrazeno 1 - 10
of 1 949
pro vyhledávání: '"Oberoi, P."'
Type-I solar noise storms are perhaps the most commonly observed active radio emissions from the Sun at meter-wavelengths. Noise storms have a long-lived and wideband continuum background with superposed islands of much brighter narrowband and short-
Externí odkaz:
http://arxiv.org/abs/2408.13465
Autor:
Maji, Moupiya, More, Surhud, Sule, Aniket, Balasubramanya, Vishaak, Bhandari, Ankit, Chand, Hum, Chavan, Kshitij, Dasgupta, Avik, De, Anindya, Gangopadhyay, Jayant, Gulati, Mamta, Hasan, Priya, Ishtiyaq, Syed, Madani, Meraj, Misra, Kuntal, N, Amoghavarsha, Oberoi, Divya, Pattnaik, Subhendu, Patwardhan, Mayuri, Ramanujam, Niruj Mohan, Ranadive, Pritesh, Sawant, Disha, Sharma, Paryag, Sharma, Twinkle, Shetye, Sai, Singhal, Akshat, Srivastava, Ajit M., Sudan, Madhu, Syed, Mumtaz, Vikranth, Pulamathi, Yadav, Virendra
We present the results of a nation-wide baseline survey, conducted by us, for the status of Astronomy education among secondary school students in India. The survey was administered in 10 different languages to over 2000 students from diverse backgro
Externí odkaz:
http://arxiv.org/abs/2406.12308
In recent years, digital platform companies have faced increasing challenges in managing customer complaints, driven by widespread consumer adoption. This paper introduces an end-to-end pipeline, named RE-GrievanceAssist, designed specifically for re
Externí odkaz:
http://arxiv.org/abs/2404.18963
We propose an end-to-end real-estate recommendation system, RE-RecSys, which has been productionized in real-world industry setting. We categorize any user into 4 categories based on available historical data: i) cold-start users; ii) short-term user
Externí odkaz:
http://arxiv.org/abs/2404.16553
Publikováno v:
ApJ 968 55 (2024)
The geo-effectiveness of coronal mass ejections (CMEs) is determined primarily by their magnetic fields. Modeling of Gyrosynchrotron (GS) emission is a promising remote sensing technique to measure the CME magnetic field at coronal heights. However,
Externí odkaz:
http://arxiv.org/abs/2404.14714
Autor:
Garg, Anupam, Raina, Aryaman, Gupta, Aryan, Singh, Jaskaran, Saini, Manav, Iiitd, Prachi, Mehta, Ronit, Oberoi, Rupin, Sharma, Sachin, Jain, Samyak, Tyagi, Sarthak, Arora, Utkarsh, Kumar, Dhruv
This study examines the use of large language models (LLMs) by undergraduate and graduate students for programming assignments in advanced computing classes. Unlike existing research, which primarily focuses on introductory classes and lacks in-depth
Externí odkaz:
http://arxiv.org/abs/2404.04603
Autor:
Zhou, Da, Pham, Yen Thi Hai, Dang, Diem Thi-Xuan, Sanchez, David, Oberoi, Aaryan, Wang, Ke, Fest, Andres, Sredenschek, Alexander, Liu, Mingzu, Terrones, Humberto, Das, Saptarshi, Le, Dai-Nam, Woods, Lilia M., Phan, Manh-Huong, Terrones, Mauricio
Monolayers of molybdenum disulfide (MoS2) are the most studied two-dimensional (2D) transition-metal dichalcogenides (TMDs), due to its exceptional optical, electronic, and opto-electronic properties. Recent studies have shown the possibility of inco
Externí odkaz:
http://arxiv.org/abs/2401.16806
Autor:
Kansabanik, Devojyoti, Mondal, Surajit, Oberoi, Divya, Chibueze, James O., Engelbrecht, N. E., Strauss, R. D., Kontar, Eduard P., Botha, Gert J. J., Steyn, P. J., Nel, Amore E.
Publikováno v:
ApJ 961 96 (2024)
Solar radio emissions provide several unique diagnostics to estimate different physical parameters of the solar corona, which are otherwise simply inaccessible. However, imaging the highly dynamic solar coronal emissions spanning a large range of ang
Externí odkaz:
http://arxiv.org/abs/2307.01895
Weak Impulsive Narrowband Quiet Sun Emissions (WINQSEs) are a newly discovered class of radio emission from the solar corona. These emissions are characterized by their extremely impulsive, narrowband and ubiquitous nature. We have systematically bee
Externí odkaz:
http://arxiv.org/abs/2306.16390
The solar corona is extremely dynamic. Every leap in observational capabilities has been accompanied by unexpected revelations of complex dynamic processes. The ever more sensitive instruments now allow us to probe events with increasingly weaker ene
Externí odkaz:
http://arxiv.org/abs/2306.15104