Zobrazeno 1 - 10
of 992
pro vyhledávání: '"A. G. Randall"'
Autor:
Postman, Marc, Lauer, Tod R., Parker, Joel W., Spencer, John R., Weaver, Harold A., Shull, J. Michael, Stern, S. Alan, Brandt, Pontus, Conard, Steven J., Gladstone, G. Randall, Lisse, Carey M., Porter, Simon D., Singer, Kelsi N., Verbiscer, Anne J.
We obtained New Horizons LORRI images to measure the cosmic optical background (COB) intensity integrated over $0.4\lesssim\lambda\lesssim0.9{~\rm\mu m}.$ The survey comprises 16 high Galactic-latitude fields selected to minimize scattered diffuse Ga
Externí odkaz:
http://arxiv.org/abs/2407.06273
Autor:
Dunn, William R., Koutroumpa, Dimitra, Carter, Jennifer A., Kuntz, Kip D., McEntee, Sean, Deskins, Thomas, Parry, Bryn, Wolk, Scott, Lisse, Carey, Dennerl, Konrad, Jackman, Caitriona M., Weigt, Dale M., Porter, F. Scott, Branduardi-Raymont, Graziella, Bodewits, Dennis, Leppard, Fenn, Foster, Adam, Gladstone, G. Randall, Parmar, Vatsal, Brophy-Lee, Stephenie, Feldman, Charly, Ness, Jan-Uwe, Cumbee, Renata, Markevitch, Maxim, Kraft, Ralph, Bogdan, Akos, Bhardwaj, Anil, Wibisono, Affelia, Mernier, Francois, Ogorzalek, Anna
The Line Emission Mapper's (LEM's) exquisite spectral resolution and effective area will open new research domains in Astrophysics, Planetary Science and Heliophysics. LEM will provide step-change capabilities for the fluorescence, solar wind charge
Externí odkaz:
http://arxiv.org/abs/2310.13873
Autor:
Mark Lutz, BA, Zhandong Zhou, MD, Ahmad Nazem, MD, G. Randall Green, MD, JD, MBA, Anton Cherney, MD, Karikehalli Dilip, MD, Charles J. Lutz, MD
Publikováno v:
JTCVS Open, Vol 21, Iss , Pp 119-121 (2024)
Externí odkaz:
https://doaj.org/article/0933a0b71eb941e99b66fb5668e753eb
Autor:
Fletcher, Leigh N., Cavalié, Thibault, Grassi, Davide, Hueso, Ricardo, Lara, Luisa M., Kaspi, Yohai, Galanti, Eli, Greathouse, Thomas K., Molyneux, Philippa M., Galand, Marina, Vallat, Claire, Witasse, Olivier, Lorente, Rosario, Hartogh, Paul, Poulet, François, Langevin, Yves, Palumbo, Pasquale, Gladstone, G. Randall, Retherford, Kurt D., Dougherty, Michele K., Wahlund, Jan-Erik, Barabash, Stas, Iess, Luciano, Bruzzone, Lorenzo, Hussmann, Hauke, Gurvits, Leonid I., Santolik, Ondřej, Kolmasova, Ivana, Fischer, Georg, Müller-Wodarg, Ingo, Piccioni, Giuseppe, Fouchet, Thierry, Gérard, Jean-Claude, Sánchez-Lavega, Agustin, Irwin, Patrick G. J., Grodent, Denis, Altieri, Francesca, Mura, Alessandro, Drossart, Pierre, Kammer, Josh, Giles, Rohini, Cazaux, Stéphanie, Jones, Geraint, Smirnova, Maria, Lellouch, Emmanuel, Medvedev, Alexander S., Moreno, Raphael, Rezac, Ladislav, Coustenis, Athena, Costa, Marc
Publikováno v:
Space Sci Rev. 2023; 219(7): 53
ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital tour tailored to maximise observing opportunities. We review the Jupit
Externí odkaz:
http://arxiv.org/abs/2304.10229
Autor:
Giles, Rohini S., Hue, Vincent, Greathouse, Thomas K., Gladstone, G. Randall, Kammer, Joshua A., Versteeg, Maarten H., Bonfond, Bertrand, Grodent, Denis G., Gérard, Jean-Claude, Sinclair, James A., Bolton, Scott J., Levin, Steven M.
Reflected sunlight observations from the Ultraviolet Spectrograph (UVS) on the Juno spacecraft were used to study the distribution of acetylene (C$_2$H$_2$) at Jupiter's south pole. We find that the shape of the C$_2$H$_2$ absorption feature varies s
Externí odkaz:
http://arxiv.org/abs/2302.10946
Publikováno v:
Frontiers in Environmental Science, Vol 12 (2024)
This study evaluated the recovery of amorphous calcium phosphate and vivianite from industrial wastewater produced by a toothpaste manufacturing facility, where phosphorus concentrations exceed 3,000 mg L−1. The goal was to reduce the phosphorus co
Externí odkaz:
https://doaj.org/article/7a0b1163682745f2897cbf56bf570790
Autor:
S. Sembay, A. L. Alme, D. Agnolon, T. Arnold, A. Beardmore, A. Belén Balado Margeli, C. Bicknell, C. Bouldin, G. Branduardi-Raymont, T. Crawford, J. P. Breuer, T. Buggey, G. Butcher, R. Canchal, J. A. Carter, A. Cheney, Y. Collado-Vega, H. Connor, N. Eaton, C. Feldman, C. Forsyth, T. Frantzen, G. Galgóczi, J. Garcia, G. Y. Genov, C. Gordillo, H-P. Gröbelbauer, M. Guedel, Y. Guo, M. Hailey, D. Hall, R. Hampson, J. Hasiba, O. Hetherington, A. Holland, S-Y. Hsieh, M. W. J. Hubbard, H. Jeszenszky, M. Jones, T. Kennedy, K. Koch-Mehrin, S. Kögl, S. Krucker, K. D. Kuntz, C. Lakin, G. Laky, O. Lylund, A. Martindale, J. Miguel Mas Hesse, R. Nakamura, K. Oksavik, N. Østgaard, H. Ottacher, R. Ottensamer, C. Pagani, S. Parsons, P. Patel, J. Pearson, G. Peikert, F. S. Porter, T. Pouliantis, B. H. Qureshi, W. Raab, G. Randall, A. M. Read, N. M. M. Roque, M. E. Rostad, C. Runciman, S. Sachdev, A. Samsonov, M. Soman, D. Sibeck, S. Smit, J. Søndergaard, R. Speight, S. Stavland, M. Steller, TianRan Sun, J. Thornhill, W. Thomas, K. Ullaland, B. Walsh, D. Walton, C. Wang, S. Yang
Publikováno v:
Earth and Planetary Physics, Vol 8, Iss 1, Pp 5-14 (2024)
The Soft X-ray Imager (SXI) is part of the scientific payload of the Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) mission. SMILE is a joint science mission between the European Space Agency (ESA) and the Chinese Academy of Sciences (CAS)
Externí odkaz:
https://doaj.org/article/6b19bd85a1e24e6fbe503471fa9df545
Autor:
Lauer, Tod R., Postman, Marc, Spencer, John R., Weaver, Harold A., Stern, S. Alan, Gladstone, G. Randall, Binzel, Richard P., Britt, Daniel T., Buie, Marc W., Buratti, Bonnie J., Cheng, Andrew F., Grundy, W. M., Horányi, Mihaly, Kavelaars, J. J., Linscott, Ivan R., Lisse, Carey M., McKinnon, William B., McNutt, Ralph L., Moore, Jeffrey M., Núñez, Jorge I., Olkin, Catherine B., Parker, Joel W., Porter, Simon B., Reuter, Dennis C., Robbins, Stuart J., Schenk, Paul M., Showalter, Mark R., Singer, Kelsi N., Verbiscer, Anne. J., Young, Leslie A.
We used New Horizons LORRI images to measure the optical-band ($0.4\lesssim\lambda\lesssim0.9{\rm\mu m}$) sky brightness within a high galactic-latitude field selected to have reduced diffuse scattered light from the Milky Way galaxy (DGL), as inferr
Externí odkaz:
http://arxiv.org/abs/2202.04273
Autor:
Giles, Rohini S., Greathouse, Thomas K., Hue, Vincent, Gladstone, G. Randall, Melin, Henrik, Fletcher, Leigh N., Irwin, Patrick G. J., Kammer, Joshua A., Versteeg, Maarten H., Bonfond, Bertrand, Grodent, Denis C., Bolton, Scott J., Levin, Steven M.
The UVS instrument on the Juno mission records far-ultraviolet reflected sunlight from Jupiter. These spectra are sensitive to the abundances of chemical species in the upper atmosphere and to the distribution of the stratospheric haze layer. We comb
Externí odkaz:
http://arxiv.org/abs/2107.11295
Autor:
Roth, Lorenz, Ivchenko, Nickolay, Gladstone, G. Randall, Saur, Joachim, Grodent, Denis, Bonfond, Bertrand, Molyneux, Philippa M., Retherford, Kurt D.
Ganymede's atmosphere is produced by charged particle sputtering and sublimation of its icy surface. Previous far-ultraviolet observations of the O{\small I\,}1356-{\AA} and O{\small I\,}1304-{\AA} oxygen emissions were used to infer sputtered molecu
Externí odkaz:
http://arxiv.org/abs/2106.03570