John Darlington (Imperial College London) - CitizenGrid

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John Darlington (Imperial College London) presenting a user-friendly crowdsourcing platform, CitizenGrid, at the Citizen Cyberlab Summit, 17-18 September 2015, University of Geneva (UNIGE).

Wissenschaft

Unified Support for Volunteer
Computing
Volunteers
(Citizens)
Resources
Local
Machine
Cloud
Credentials
Thinking
Local
(VBox)
Cloud
Game
Developers
(Scientists)
Register
Games
Local (Vbox)
Cloud (EC2,
Openshare)
CitizenGrid

Volunteers
(App Users)
CitizenGrid
VBox VMI
Cloud VMI
Location
Details
Cloud
Credentials
VM on
OpenStack
VM on
AWS
VM on
VBox
CCS
Applications
Directory Launch the
App
VC
Application
VT
Application
Launch the
App
Browser
Register and
Login
Add Cloud
Credentials
Search and
Select a CCS
Application
Support for Volunteers

CitizenGrid Features
John Darlington & Poonam Yadav – ICSTM
User Account
Management
Sign-up, Login/log out
Account update /Password
recovery
User role switch facility
Application Group Management
Online
Resources
& REstFul
API
Help-guide and
documentation
Browse-able public API
Source code: Github
public repository
Application
Management
Application creation
wizard
Application tagging
(Branches, Categories)
Virtual Box image
upload
Cloud Image’s info
registration
Applications and images
delete facility
Cloud
Credential
Management
OpenStack and EC2
cloud credentials
Add credentials
Delete credentials
Application
Server and
Client
hosting on
Cloud
Launching of VM
instances on
EC2/OpenStack
Running-Instance
status check
Stopping a running
instance
Application
Portal with
free text
search
Table view of public
registered applications
Free text based search
on applications
Ordered view of
applications
Detail view of selected
application with
launching facility
Application
Client
Launch on
Local Virtual
Box
Launches Vbox images on
local Vbox
Provides support for both
x86 and x86_64
Provides support for Ubuntu
and other Linux versions

Cyberlab pilot Projects and Tools
CERN VM with copilot (LHC@home 2.0)
CERN VAS Game
Redwire
EpiCollect
GeoKey

CitizenGrid, VAS & LiveQ
VAS Game
LHC
Volunteer
Computing
Infrastructure
VAS Game
Players
CitizenGrid
Citizen
Science
Volunteers
ProjectCreatorTeam
VAS worker node
VAS Worker
Node on Local VBox
VAS Worker
Node on a Cloud
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The highest priority recommendation of the Astro2020 Decadal Survey for space-based astronomy was the construction of an observatory capable of characterizing habitable worlds. In this paper series we explore the detectability of and interference from exomoons and exorings serendipitously observed with the proposed Habitable Worlds Observatory (HWO) as it seeks to characterize exoplanets, starting in this manuscript with Earth-Moon analog mutual events. Unlike transits, which only occur in systems viewed near edge-on, shadow (i.e., solar eclipse) and lunar eclipse mutual events occur in almost every star-planet-moon system. The cadence of these events can vary widely from ∼yearly to multiple events per day, as was the case in our younger Earth-Moon system. Leveraging previous space-based (EPOXI) lightcurves of a Moon transit and performance predictions from the LUVOIR-B concept, we derive the detectability of Moon analogs with HWO. We determine that Earth-Moon analogs are detectable with observation of ∼2-20 mutual events for systems within 10 pc, and larger moons should remain detectable out to 20 pc. We explore the extent to which exomoon mutual events can mimic planet features and weather. We find that HWO wavelength coverage in the near-IR, specifically in the 1.4 µm water band where large moons can outshine their host planet, will aid in differentiating exomoon signals from exoplanet variability. Finally, we predict that exomoons formed through collision processes akin to our Moon are more likely to be detected in younger systems, where shorter orbital periods and favorable geometry enhance the probability and frequency of mutual events.

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Cyanobacteria (also known as blue-green algae) are ubiquitous photosynthetic microorganisms found in diverse habitats such as fresh water, marine water, moist rocks, etc. The photosynthetic mode of nutrition makes them significant global oxygen producers along with nitrogen-fixing ability of heterocyst and carbon sequestration. Some cyanobacterial species have the ability to perform a dual mode of nutritional procurement. This unique capability of cyanobacteria to utilize both organic (heterotrophic) and inorganic (autotrophic) carbon sources for energy production and growth is termed as mixotrophy which impart nutritional flexibility and competitive ability to them. Cyanobacterial mixotrophy provides the promising avenues in biotechnological applications such as wastewater treatment, bioremediation, pharmaceuticals, food supplements, biofertilizer, coloring agents, synthesis of bioactive compounds and as an agent for eco-friendly bio-fuels generation, etc Mixotrophically grown cyanobacteria, demonstrate significant potential for efficient and economical applications beyond their conventional agricultural application, thereby offering a versatile and impactful resource for future technological and environmental challenges.

mixotrophy in cyanobacteria: a dual nutritional strategy

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Hadean zircons provide a potential record of Earth's earliest subduction 4.3 billion years ago. Itremains enigmatic how subduction could be initiated so soon after the presumably Moon‐forming giant impact(MGI). Earlier studies found an increase in Earth's core‐mantle boundary (CMB) temperature due to theaccumulation of the impactor's core, and our recent work shows Earth's lower mantle remains largely solid, withsome of the impactor's mantle potentially surviving as the large low‐shear velocity provinces (LLSVPs). Here,we show that a hot post‐impact CMB drives the initiation of strong mantle plumes that can induce subductioninitiation ∼200 Myr after the MGI. 2D and 3D thermomechanical computations show that a high CMBtemperature is the primary factor triggering early subduction, with enrichment of heat‐producing elements inLLSVPs as another potential factor. The models link the earliest subduction to the MGI with implications forunderstanding the diverse tectonic regimes of rocky planets.

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PESTS OF SUGARCANE - BORERS BORERS 1. Early shoot borer, Chilo infuscatellus, Crambidae, Lepidoptera Symptom of damage: Deadheart in 1-3 month old crop, which can be easily pulled out, rotten portion of the straw coloured dead-heart emits an offensive odour. A number of bore holes at the base of the shoot just above the ground level. Nature of damage: Caterpillar bores into the central shoot and feeds on the internal tissue. This cause interference in the translocation of plant sap and damage the sugar storing tissues. Egg: Flat-scale like eggs are laid in 3-5 rows on the lower surface of leaves in masses of 4-100. The masses are slightly overlapping like tiles. Larva: Larva is dirty white with five dark violet longitudinal stripes and dark brown head. Pupa: Pupation takes place within the tunnel. Caterpillar before pupating makes a large exit hole in the stem and blocks the opening with silken discs. Adult: Pale greyish brown moth with black dots near the costal margin of the forewings and with white hindwings. 2. Internode borer, Chilo sacchariphagus indicus, Crambidae, Lepidoptera Symptom of damage: Internodes constricted and shortened, with a number of boreholes and fresh excreta in the nodal region. Affected tissues reddened. Nature of damage: Caterpillars attack sugarcane plants after 3 months of planting. They bore into the canes near the nodes; entry holes are plugged with excreta. Entry is generally confined to the first five internodes. Egg: Scale-like white eggs are laid by female moths in batches of 9-11, near the midribs, on leaf sheaths or on stem. Larva: White larva with four violet longitudinal stripes and light brown head. Pupa: Pupation takes place in semi-dried leaf sheath. Adult: Pale brown with white hind wings. 3. Top borer, Scirpophaga excerptalis, Pyralidae, Lepidoptera Symptom of damage: Deadheart in grownup canes, which cannot be easily pulled; deadheart reddish brown in colour; parallel row of shot holes in the emerging leaves and red tunnels in the midribs of leaves; bunchy tip due to the growth of side shoots. Nature of damage: Caterpillars are mainly found in the apical portion of the canes, boring through the growing point and down the upper joints until it reaches the sappy portion of the stem, there it feeds on the tissues and destroys the cane. They also bore into the unfolded leaves preferably into the midrib, mining its way to the base. Egg: Eggs are laid on the lower surface of top leaves in clusters particularly near midribs. The clusters are covered with buff coloured hairs. Larva :Smooth, white or cream coloured with a red coloured mid-dorsal line and yellow head. Pupa: Pupation takes place within the larval tunnel in a chamber with an exit hole constructed by the caterpillar. Adult: White coloured moth (with a buff coloured anal tuft in the abdominal tip of female).

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In this work, we assess the potential detectability of solar panels made of silicon on an Earth-like exoplanet as a potential technosignature. Silicon-based photovoltaic cells have high reflectance in the UV-VIS and in the near-IR, within the wavelength range of a space-based flagship mission concept like the Habitable Worlds Observatory (HWO). Assuming that only solar energy is used to provide the 2022 human energy needs with a land cover of ∼ 2.4%, and projecting the future energy demand assuming various growth-rate scenarios, we assess the detectability with an 8 m HWO-like telescope. Assuming the most favorable viewing orientation, and focusing on the strong absorption edge in the ultraviolet-to-visible (0.34 − 0.52 µm), we find that several 100s of hours of observation time is needed to reach a SNR of 5 for an Earth-like planet around a Sun-like star at 10pc, even with a solar panel coverage of ∼ 23% land coverage of a future Earth. We discuss the necessity of concepts like Kardeshev Type I/II civilizations and Dyson spheres, which would aim to harness vast amounts of energy. Even with much larger populations than today, the total energy use of human civilization would be orders of magnitude below the threshold for causing direct thermal heating or reaching the scale of a Kardashev Type I civilization. Any extraterrrestrial civilization that likewise achieves sustainable population levels may also find a limit on its need to expand, which suggests that a galaxy-spanning civilization as imagined in the Fermi paradox may not exist.

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ANONYMOUS

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SELF-EXPLANATORY

Mammals have dominated Earth for approximately 55 Myr thanks to their adaptations and resilience to warming and cooling during the Cenozoic. All life will eventually perish in a runaway greenhouse once absorbed solar radiation exceeds the emission of thermal radiation in several billions of years. However, conditions rendering the Earth naturally inhospitable to mammals may develop sooner because of long-term processes linked to plate tectonics (short-term perturbations are not considered here). In ~250 Myr, all continents will converge to form Earth’s next supercontinent, Pangea Ultima. A natural consequence of the creation and decay of Pangea Ultima will be extremes in pCO2 due to changes in volcanic rifting and outgassing. Here we show that increased pCO2, solar energy (F⨀; approximately +2.5% W m−2 greater than today) and continentality (larger range in temperatures away from the ocean) lead to increasing warming hostile to mammalian life. We assess their impact on mammalian physiological limits (dry bulb, wet bulb and Humidex heat stress indicators) as well as a planetary habitability index. Given mammals’ continued survival, predicted background pCO2 levels of 410–816 ppm combined with increased F⨀ will probably lead to a climate tipping point and their mass extinction. The results also highlight how global landmass configuration, pCO2 and F⨀ play a critical role in planetary habitability.

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John Darlington (Imperial College London) - CitizenGrid

1. Imperial College London

2. Unified Support for Volunteer Computing Volunteers (Citizens) Resources Local Machine Cloud Credentials Thinking Local (VBox) Cloud Game Developers (Scientists) Register Games Local (Vbox) Cloud (EC2, Openshare) CitizenGrid

3. Support for Scientists

4. Volunteers (App Users) CitizenGrid VBox VMI Cloud VMI Location Details Cloud Credentials VM on OpenStack VM on AWS VM on VBox CCS Applications Directory Launch the App VC Application VT Application Launch the App Browser Register and Login Add Cloud Credentials Search and Select a CCS Application Support for Volunteers

5. CitizenGrid Features John Darlington & Poonam Yadav – ICSTM User Account Management Sign-up, Login/log out Account update /Password recovery User role switch facility Application Group Management Online Resources & REstFul API Help-guide and documentation Browse-able public API Source code: Github public repository Application Management Application creation wizard Application tagging (Branches, Categories) Virtual Box image upload Cloud Image’s info registration Applications and images delete facility Cloud Credential Management OpenStack and EC2 cloud credentials Add credentials Delete credentials Application Server and Client hosting on Cloud Launching of VM instances on EC2/OpenStack Running-Instance status check Stopping a running instance Application Portal with free text search Table view of public registered applications Free text based search on applications Ordered view of applications Detail view of selected application with launching facility Application Client Launch on Local Virtual Box Launches Vbox images on local Vbox Provides support for both x86 and x86_64 Provides support for Ubuntu and other Linux versions

7. Cyberlab pilot Projects and Tools CERN VM with copilot (LHC@home 2.0) CERN VAS Game Redwire EpiCollect GeoKey

8. CitizenGrid, VAS & LiveQ VAS Game LHC Volunteer Computing Infrastructure VAS Game Players CitizenGrid Citizen Science Volunteers ProjectCreatorTeam VAS worker node VAS Worker Node on Local VBox VAS Worker Node on a Cloud 1 2 3 4 5 6 7 8 9 10

Hinweis der Redaktion

User Account Management: sign-up, login, password recovery, user account update facility, user role switch facility. Online Resources: User Help-guide and documentation, browse- able public API. Application Management: Multi-page application creation, application tagging (Branches/Categories/subcategories), Virtual Box Image upload for application client ( compressed or uncompressed), Cloud Images details registration for application’s client and server, Application delete functionality. Cloud Credential Management: Openstack and EC2 credential management (Add, Delete). Application Hosting on Cloud: Support for launching, status check and stopping on VM instances of application’s server and client on OpenStack and EC2. Application Client Launch on Virtual Box: Support of launching application client on local VirtualBox. Applications Search Portal: Public registered applications search portal where applications can be search based on free text or in field order.

John Darlington (Imperial College London) - CitizenGrid

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