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Tämä raportti on koottu haastatteluista, joita tehtiin 13:ssa Kotkan–Haminan seudulla toimivassa matkailualan yrityksessä keväällä 2015. Toimialoina olivat matkailun ohjelmapalvelut (viisi), museot (kolme), hotellit (kolme) ja matkanjärjestäjät (kaksi yritystä). Haastatteluissa yrityksiltä kysyttiin, mitä ammattiryhmiä heillä työskentelee ja mitä tietoja ja taitoja heiltä tällä hetkellä työssään edellytetään. Toinen kysymys ennakoi tilannetta 3 - 5 vuoden päästä: Mitkä osaamiset tulevaisuudessa korostuvat? Mitä aivan uutta osaamista tullaan tarvitsemaan? Kolmas teema liittyi sellaiseen osaamiseen, jota yrityksessä pitäisi välittömästi kehittää. Osaamiskartoitus toteutettiin C&Q-järjestelmällä ja Uudenmaan ELY-keskuksen rahoittaman Tykenelikko2-hankkeen tuella. Raporttia on täydennetty vuonna 2012 haastatelluissa seudun ravintoloissa (viisi yritystä) esiin nousseilla osaamistarpeilla.
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Theoretical predictions and observational data indicate a class of sub-Neptune exoplanets may have water-rich interiors covered by hydrogen-dominated atmospheres. Provided suitable climate conditions, such planets could host surface liquid oceans. Motivated by recent JWST observations of K2-18 b, we self-consistently model the photochemistry and potential detectability of biogenic sulfur gases in the atmospheres of temperate sub-Neptune waterworlds for the first time. On Earth today, organic sulfur compounds produced by marine biota are rapidly destroyed by photochemical processes before they can accumulate to significant levels. Domagal-Goldman et al. suggest that detectable biogenic sulfur signatures could emerge in Archean-like atmospheres with higher biological production or low UV flux. In this study, we explore biogenic sulfur across a wide range of biological fluxes and stellar UV environments. Critically, the main photochemical sinks are absent on the nightside of tidally locked planets. To address this, we further perform experiments with a 3D general circulation model and a 2D photochemical model (VULCAN 2D) to simulate the global distribution of biogenic gases to investigate their terminator concentrations as seen via transmission spectroscopy. Our models indicate that biogenic sulfur gases can rise to potentially detectable levels on hydrogen-rich water worlds, but only for enhanced global biosulfur flux (20 times modern Earth’s flux). We find that it is challenging to identify DMS at 3.4 μm where it strongly overlaps with CH4, whereas it is more plausible to detect DMS and companion byproducts, ethylene (C2H4) and ethane (C2H6), in the mid-infrared between 9 and 13 μm. Unified Astronomy Thesaurus concepts: Exoplanet atmospheres (487); Exoplanet
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
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Sérgio Sacani
Basic concept of chemistry
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Areesha Ahmad
This presentation offers the bird's eye view of the cell as the basic structural and functional unit of life. It also addresses the origin of eukaryotic cells from the prokaryotic cell by the endosymbiotic theory.
CELL -Structural and Functional unit of life.pdf
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COST ESTIMATION FOR A RESEARCH PROJECT.pptx
COST ESTIMATION FOR A RESEARCH PROJECT.pptx
Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds
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GBSN - Biochemistry (Unit 1)
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CELL -Structural and Functional unit of life.pdf
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module for grade 9 for distance learning
module for grade 9 for distance learning
Boyle’s Law
1.
Group Member :- huzair Afiq Faizah fatana
2.
Boyle’s Law Robert Boyle
1621-1691
3.
What is the
Definition?
4.
Boyle’s Law Defined Temperature
is constant Volume occupied by a gas varies inversely with the applied pressure
5.
Boyle’s law Equation
6.
An animation showing the relationship
between pressure and volume when amount and temperature are held constant
7.
Pressure Volume
8.
Pressure Volume
9.
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