Search Results - "Noci, G."

Ultraviolet Coronagraph Spectrometer Observations of Density Fluctuations in the Solar Wind by Ofman, L, Romoli, M, Poletto, G, Noci, G, Kohl, J. L

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SMART-1 mission to the Moon: Status, first results and goals by Foing, B.H., Racca, G.D., Marini, A., Evrard, E., Stagnaro, L., Almeida, M., Koschny, D., Frew, D., Zender, J., Heather, J., Grande, M., Huovelin, J., Keller, H.U., Nathues, A., Josset, J.L., Malkki, A., Schmidt, W., Noci, G., Birkl, R., Iess, L., Sodnik, Z., McManamon, P.

“…We present the first results from SMART-1’s science and technology payload. SMART-1 is Europe’s first lunar mission and will provide some significant advances…”
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UVCS/SOHO Empirical Determinations of Anisotropic Velocity Distributions in the Solar Corona by Kohl, J. L, Noci, G, Antonucci, E, Tondello, G, Huber, M. C. E, Cranmer, S. R, Strachan, L, Panasyuk, A. V, Gardner, L. D, Romoli, M, Fineschi, S, Dobrzycka, D, Raymond, J. C, Nicolosi, P, Siegmund, O. H. W, Spadaro, D, Benna, C, Ciaravella, A, Giordano, S, Habbal, S. R, Karovska, M, Li, X, Martin, R, Michels, J. G, Modigliani, A, Naletto, G, O'Neal, R. H, Pernechele, C, Poletto, G, Smith, P. L, Suleiman, R. M

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UVCS WLC Observations of Compressional Waves in the South Polar Coronal Hole by Ofman, L, Romoli, M, Poletto, G, Noci, G, Kohl, J. L

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Identification of the Coronal Sources of the Fast Solar Wind by Giordano, S, Antonucci, E, Noci, G, Romoli, M, Kohl, J. L

“…The present spectroscopic study of the ultraviolet coronal emission in a polar hole, detected on 1996 April 6-9 with the Ultraviolet Coronagraph Spectrometer…”
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An Empirical Model of a Polar Coronal Hole at Solar Minimum by Cranmer, S. R, Kohl, J. L, Noci, G, Antonucci, E, Tondello, G, Huber, M. C. E, Strachan, L, Panasyuk, A. V, Gardner, L. D, Romoli, M, Fineschi, S, Dobrzycka, D, Raymond, J. C, Nicolosi, P, Siegmund, O. H. W, Spadaro, D, Benna, C, Ciaravella, A, Giordano, S, Habbal, S. R, Karovska, M, Li, X, Martin, R, Michels, J. G, Modigliani, A, Naletto, G, O'Neal, R. H, Pernechele, C, Poletto, G, Smith, P. L, Suleiman, R. M

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Two-dimensional Structure of a Polar Coronal Hole at Solar Minimum: New Semiempirical Methodology for Deriving Plasma Parameters by Zangrilli, L, Poletto, G, Nicolosi, P, Noci, G, Romoli, M

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First Results from the Soho Ultraviolet Coronagraph Spectrometer by Kohl, J L, Noci, G, Antonucci, E, Tondello, G, Huber, M C; E, Gardner, L D, Nicolosi, P, Strachan, L, Fineschi, S, Raymond, J C, Romoli, M, Spadaro, D, Panasyuk, A, Siegmund, O H; W, Benna, C, Ciaravella, A, Cranmer, S R, Giordano, S, Karovska, M, Martin, R, Michels, J, Modigliani, A, Naletto, G, Pernechele, C, Poletto, G, Smith, P L

“…The SOHO Ultraviolet Coronagraph Spectrometer (UVCS/SOHO) is being used to observe the extended solar corona from 1.25 to 10 R from Sun center. Initial…”
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Origins of the Slow and the Ubiquitous Fast Solar Wind by Habbal, S. R, Woo, R, Fineschi, S, O'Neal, R, Kohl, J, Noci, G, Korendyke, C

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Composition of Coronal Streamers from the SOHO Ultraviolet Coronagraph Spectrometer by Raymond, J C, Kohl, J L, Noci, G, Antonucci, E, Tondello, G, Huber, MCE, Gardner, L D, Nicolosi, P, Fineschi, S, Romoli, M, Spadaro, D, Siegmund, OHW, Benna, C, Ciaravella, A, Cranmer, S, Giordano, S, Karovska, M, Martin, R, Michels, J, Modigliani, A, Naletto, G, Panasyuk, A, Pernechele, C, Poletto, G, Smith, Peter L, Suleiman, R M, Strachan, L

“…The Ultraviolet Coronagraph Spectrometer on the SOHO satellite covers the 940-1350 Å range as well as the 470-630 Å range in second order. It has detected…”
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Solar and Heliospheric Observatory Observations of a Helical Coronal Mass Ejection by Ciaravella, A, Raymond, J. C, Thompson, B. J, van Ballegooijen, A, Strachan, L, Li, J, Gardner, L, O’Neal, R, Antonucci, E, Kohl, J, Noci, G

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EUV Spectral Line Profiles in Polar Coronal Holes from 1.3 to 3.0 R by Kohl, J. L, Esser, R, Cranmer, S. R, Fineschi, S, Gardner, L. D, Panasyuk, A. V, Strachan, L, Suleiman, R. M, Frazin, R. A, Noci, G

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Physical Structure of a Coronal Streamer in the Closed-Field Region as Observed from UVCS/SOHO and SXT/Yohkoh by Li, J, Raymond, J. C, Acton, L. W, Kohl, J. L, Romoli, M, Noci, G, Naletto, G

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At last we are creating environmental strategies which work by Azzone, Giovanni, Bertelè, Umberto, Noci, Giuliano

“…Organizations face a variety of pressures leading executives to view environmental issues as an important element in their business decisions. The objective of…”
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Flexible variable-specific-impulse electric propulsion systems for planetary missions by Chesta, E., Estublier, D., Fallis, B., Gengembre, E., Gonzalez del Amo, J., Kutufa, N., Nicolini, D., Saccoccia, G., Casalino, L., Dumazert, P., Prioul, M., Boeuf, J.P., Bouchoule, A., Wallace, N., Noci, G., Berti, M., Saverdi, M., Biagioni, L., Marcuccio, S., Cadiou, A., Darnon, F., Jolivet, L.

“…Variable-specific-impulse electric propulsion systems can provide important advantages and cost reductions to any scale of planetary mission. The first part of…”
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Ultraviolet Coronagraph Spectrometer Observation of the 1996 December 23 Coronal Mass Ejection by Ciaravella, A, Raymond, J. C, Fineschi, S, Romoli, M, Benna, C, Gardner, L, Giordano, S, Michels, J, O'Neal, R, Antonucci, E, Kohl, J, Noci, G

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SMART-1 mission to the moon: Technology and science goals by Foing, B.H., Racca, G.D., Marini, A., Heather, D.J., Koschny, D., Grande, M., Huovelin, J., Keller, H.U., Nathues, A., Josset, J.L., Malkki, A., Schmidt, W., Noci, G., Birkl, R., Iess, L., Sodnik, Z., McManamon, P.

“…SMART-1 is a technology demonstration mission for deep space solar electrical propulsion and Technologies for the Future. SMART-1 will be Europe's first lunar…”
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Solar Wind at 6.8 Solar Radii from UVCS Observation of Comet C/1996Y1 by Raymond, John C, Fineschi, S, Smith, P. L, Gardner, L, O'Neal, R, Ciaravella, A, Kohl, J. L, Marsden, B, Williams, G. V, Benna, C, Giordano, S, Noci, G, Jewitt, D

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Plasma diagnostics and simulation for the SMART-1 mission by Tajmar, M, González, J, Saccoccia, G, Noci, G, Laakso, H

“…SMART-1 is a technology demonstrator for using primary electric propulsion on interplanetary spacecraft. Hence, studying of the interaction of the plasma…”
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Lyman α intensities in a polar coronal hole from a 2D model by Zangrilli, L., Poletto, G., Nicolosi, P., Noci, G.

“…We simulate the coronal H I Lyman α intensity for heliocentric distances between 1.5 and 2.5 R ⊙, and latitudes between 90° (North pole) and 30°, making use of…”
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