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We present the result of a new VLA HI Imaging survey of Virgo galaxies, VIVA(the VLA Imaging survey of Virgo galaxies in Atomic gas). The survey includeshigh resolution HI data of 53 carefully selected late type galaxies (48 spiralsand 5 irregular systems). The goal is to study environmental effects on HI gasproperties of cluster galaxies to understand which physical mechanisms affectgalaxy evolution in different density regions, and to establish how far out theimpact of the cluster reaches. As a dynamically young cluster, Virgo containsexamples of galaxies experiencing a variety of environmental effects. Itsnearness allows us to study each galaxy in great detail. We have selected Virgogalaxies with a range of star formation properties in low to high densityregions (at the projected distance from M87, d_87=0.3-3.3 Mpc). Contrary to previous studies, more than half of the galaxies in the sample (~60%) are fainterthan 12 mag in B_T. Overall, the selected galaxies represent the late typeVirgo galaxies (S0/a to Sd/Irr) down to m_p<~14.6 fairly well in morphologicaltype, systemic velocity, subcluster membership, HI mass and deficiency. In thispaper (VIVA I: the atlas and the HI properties), we present HI maps andproperties, and describe the HI morphology and kinematics of individualgalaxies in detail (abbreviated).

VIVA, VLA Imaging of Virgo spirals in Atomic gas: I. The Atlas & The HI Properties