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1by L. ZANGRILLI, G. POLETTO, G. Noci, NICOLOSI, PIERGIORGIO“...We simulate the coronal H I Lyman alpha intensity for heliocentric distances between 1.5 and 2.5 R...”
Published in Advances in Space Research (2002)
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2by Tubiana, C., Snodgrass, C., Mottola, S., Vincent, J. B., Lara, L., Fornasier, S., Knollenberg, J., Thomas, N., Fulle, M., Agarwal, J., Bodewits, D., Güttler, C., Gutierrez, P. J., Lowry, S., Oklay, N., Rodrigo, R., Sierks, H., A’Hearn, M. F., Barucci, M. A., Bertaux, J. L., Cremonese, G., Da Deppo, V., Davidsson, B., De Cecco, M., Groussin, O., Hviid, S. F., Ip, W., Jorda, L., Keller, H. U., Koschny, D., Kramm, R., Kührt, E., Küppers, M., Lamy, P. L., Lopez Moreno, J. J., Michalik, H., Rickman, H., Sabau, L., Wenzel, K. P., BERTINI, IVANO, FERRI, FRANCESCA, LA FORGIA, FIORANGELA, MAGRIN, SARA, PAJOLA, MAURIZIO, ANGRILLI, FRANCESCO, BARBIERI, CESARE, DEBEI, STEFANO, LAZZARIN, MONICA, MARZARI, FRANCESCO, NALETTO, GIAMPIERO“... photometry, we investigated how the comet brightness varies with heliocentric distance. 67P was likely...”
Published in Astronomy & Astrophysics (2015)
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3by ZANGRILLI L., POLETTO G., NOCI G., ROMOLI M., NICOLOSI, PIERGIORGIO“... with a two-dimensional semiempirical coronal hole model, for heliocentric distances between 1.4 and 2.6 R...”
Published in The Astrophysical Journal (2002)
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