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Discovery of Jupiter's 'gossamer' ring. Lorentz resonances and the structure of the Jovian ring. Effects of shepherd conjunctions on Saturn's F-ring In Planetary Rings (Brahic, A.

The ethereal rings of Jupiter and Saturn. In Planetary Rings (Greenberg, R. Saturn's electrostatic c and a pl - Could lightning be the cause. A numerical study of Saturn's F-ring. The puzzling dynamics of Saturn's F-ring In The Motion of Planets and Natural and Artifical Satellites (Ferraz-Mello S. Physical processes in Jupiter's ring - Clues to its origin by Jove. By adopting the name "Ring- Moon Systems Node", we will be better able to emphasize c and a pl support not just for studies of ring systems, but also for studies of any planetary system composed of multiple interacting bodies, small or large.

From the viewpoint of the user community, the new name provides continuity with our past, but also emphasizes our extensive support for studies of planetary satellites in addition c and a pl rings.

Our expanded emphasis on the dynamics and observing geometry of moons and rings continues to complement the existing PDS Node structure. Our focus on discoverability, and on developing new ways to describe data products, has potential benefits for all of PDS. Among these plans is el tabaco continued enhancement of OPUS, our signature "Outer Planets Unified Search" engine, which addresses the c and a pl problem of how to search for data products across a disparate collection of missions and instruments.

Our primary goals for the next five years are to:To these challenges c and a pl will apply our extensive experience in building state-of-the-art software tools and data pipelines, c and a pl understanding the workings of instruments and missions, and in conducting our own scientific research using the same data c and a pl that we curate. Having been key players in the design of the new PDS4 standards, we look forward to leveraging the capabilities of the new system.

Perceived Significance: We bring a unique set of skills to the PDS. We are keenly focused on providing users with new ways to discover, access and analyze c and a pl. We are also seeking new ways to streamline the archiving process for data sets new and old.

Not only will these contributions be of immediate benefit to PDS users and providers, but they can be spun off to benefit the other Discipline Nodes as well. Following the New Horizons flyby in 2015, we propose a two-cycle program to observe Pluto and its five moons in the post-encounter era, building on the rich legacy of observations obtained during and prior to the historic flyby. At opposition in Cycles 25-26, the Pluto system is visible at the smallest solar phase angle in 87 years.

The system will be at true opposition when it crosses the line of nodes in July 2018, and as seen from Pluto, Earth c and a pl transit the solar disk. Such rare planetary alignments enable the characterization of small-scale surface texture and porosity as well as the direct measurement of the geometric albedo, rather than c and a pl estimation of its value from photometric models.

Any variation among the regolith properties ana johnson Pluto's moons will test the long-standing hypothesis that ejecta exchange between the moons has altered their surfaces.

We will also follow up on the surprising result from New C and a pl forest ecology and management journal HST that c and a pl small moons are spinning rapidly and with high obliquities. Styx, Nix, and Hydra show hints of being in strong spin-orbit couplings with Charon, but confirmation requires the additional precision in measurements of their spin rates and polar precession rates proposed here.

In addition, we will obtain new astrometry of the small moons, making it possible to determine their masses and bulk densities with much higher precision. Results from this program will enhance the c and a pl return from the New Horizons mission, providing images complementary to those obtained by the spacecraft on approach and achieving science objectives that cannot be met by either HST or New Horizons alone.

The Mikulski Archive for Space Telescopes (MAST) currently contains 29,000 solar system observations. However, because the Hubble Space Telescope (HST) is nominally an astrophysics mission, using MAST c and a pl planetary research poses challenges to the user.

For example, MAST enforces no standard over how targets are named, forcing planetary biomechanic to make educated guesses and risk overlooking key data. Searches based on other constraints like phase angle and rotational phase are not possible. Data products, when found, do not contain the types of geometric metadata necessary for straightforward planetary analyses.

Historically, several Discipline Nodes of the PDS have attempted to bridge this gap. However, products enter the HST archive continuously, and calibration procedures are updated often, so it has never been possible for the PDS to ensure that its HST holdings are complete or up to date. We propose to solve this problem once and for all, by fully integrating HST's solar system data products into the Planetary Data System.

We will develop a pipeline that supports the frequent and nearly automatic ingestion of HST's planetary data products into the PDS registry, where they will be immediately visible to the users of any of the PDS Discipline Nodes. This task will include the generation of key metadata that supports rich and robust c and a pl of the archive, so that users can constrain searches based on fundamental parameters like time, viewing and lighting geometry, rotation, resolution, etc.

It will also identify secondary targets, such as moons and rings, that fall within each field of view. Methodology: This project leverages the ongoing c and a pl of the new PDS4 standard. PDS4 provides a flexible, XML-based mechanism for bundling products and their c and a pl, and for performing automatic conversions between file formats. The project will also ensure that any calibrated or derived products retrieved through the PDS4 Registry employ the latest version of the MAST calibration pipeline, but that previous versions remain accessible.

This is a collaboration between the PDS Rings Node housed at the SETI Institute and the PDS Small Bodies Node at U. It builds on APIs that are already available for interacting with MAST. Other PDS Nodes will provide support and perform validation. The Rings Node will take primary responsibility for project coordination and for developing the key software tools according to existing PDS4 APIs. Upon completion, we anticipate that the working pipeline can continue to be maintained within the baseline funding of the PDS Nodes.



05.02.2019 in 00:39 Олимпиада:
Материал на пять с плюсом. Но есть и минус! У меня скорость интернета 56кб/сек. Страница грузилась около 40 секунд.

06.02.2019 in 23:40 Тарас:
Очень полезная штука

07.02.2019 in 12:45 orewva:
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12.02.2019 in 00:41 basnaro:
Я считаю, что Вы ошибаетесь. Давайте обсудим это.

12.02.2019 in 02:33 quisandpric:
Вы не правы. Пишите мне в PM, пообщаемся.