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ʜᴇʀᴇ ᴡᴇ ᴀʀᴇ ᴏɴ ᴀ ᴘᴇʀꜰᴇᴄᴛ ɴɪɢʜᴛ

ᴛʜᴇ ꜱᴋʏ ɪꜱ ᴄʟᴇᴀʀ ᴀɴᴅ ᴛʜᴇ ᴍᴏᴏɴ ɪꜱ ꜰᴜʟʟ

ʟᴏᴏᴋɪɴɢ ᴏᴜᴛ ᴀᴛ ᴛʜᴇ ᴜɴɪᴠᴇʀꜱᴇ

ɪ ᴛʜᴀɴᴋ ᴛʜᴇ ꜱᴛᴀʀꜱ ᴀɴᴅ ᴛʜᴇ ʜᴇᴀᴠᴇɴꜱ ꜰᴏʀ ʏᴏᴜ

 

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Servizio di pulizia e controllo della linea per la D445.1145

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Somewhere off the Coastal Hwy 1

La D345.1145 percorre il falso doppio binario fra la stazione di Rocchetta e l'adiacente punto di diramazione fra la linea in esercizio per Potenza ed il tronco di quella per Spinazzola ancor oggi in esercizio quale raccordo per il polo industriale di San Nicola di Melfi al traino del convoglio FIAT da Torino Orbassano. (20/11/14)

 

The D345.1145 hauls the FIAT train from Turin to San Nicola di Melfi on the short part of the Foggia-Spinazzola line between the station of Rocchetta and the freight yard in San Nicola.

The first track is however the one of the Foggia-Potenza line. (2014-11-20)

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La famosa D445.1145 della discordia impegnata sulla Sulmona - Castel di Sangro per pulizia linea, qui ripresa nei pressi della stazione di Palena, sullo sfondo l'imponente massiccio della Majella.

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La d445.1145 al traino del su treno speciale diretto a Isernia.

One of many unsufficient attempts to capture the vastness of the pampas from behind the window of a bus.

La D445.1145 in transito nei pressi del segnale ad ala di Roccaraso di ritorno vetrso Sulmona.

Happy 4th of July

Cardinal in blooming ornamental pear tree.

   

El cotxe 1145 de Avanza Baix és un dels quatre MAN NG313F amb carrosseria Castrosua CS40 procedents de la flota de TMB. A la fotografia veiem el 3428 de TMB renumerat 1145, circulant a la linia L94.

LOCATION : Batalha, Portugal

Fondazione FS Sulmona-Rivisondoli/Pescocostanzo

The events surrounding the Big Bang were so cataclysmic that they left an indelible imprint on the fabric of the cosmos. We can detect these scars today by observing the oldest light in the universe. As it was created nearly 14 billion years ago, this light — which exists now as weak microwave radiation and is thus named the cosmic microwave background (CMB) — permeates the entire cosmos, filling it with detectable photons.

 

The CMB can be used to probe the cosmos via something known as the Sunyaev-Zel’dovich (SZ) effect, which was first observed over 30 years ago. We detect the CMB here on Earth when its constituent microwave photons travel to us through space. On their journey to us, they can pass through galaxy clusters that contain high-energy electrons. These electrons give the photons a tiny boost of energy. Detecting these boosted photons through our telescopes is challenging but important — they can help astronomers to understand some of the fundamental properties of the universe, such as the location and distribution of dense galaxy clusters.

 

The NASA/ESA (European Space Agency) Hubble Space Telescope observed one of most massive known galaxy clusters, RX J1347.5–1145, seen in this Picture of the Week, as part of the Cluster Lensing And Supernova survey with Hubble (CLASH). This observation of the cluster, 5 billion light-years from Earth, helped the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile to study the cosmic microwave background using the thermal Sunyaev-Zel’dovich effect. The observations made with ALMA are visible as the blue-purple hues.

 

Image credit: ESA/Hubble & NASA, T. Kitayama (Toho University, Japan)/ESA/Hubble & NASA

 

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NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.

 

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Raven Meadows bus park, Shrewsbury

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