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Spatial distribution and ecological risk of heavy metals and their source apportionment in soils from a typical mining area, Inner Mongolia, China
Determining the distributions and sources of heavy metals in soils and assessing ecological risks are fundamental tasks in the control and management...
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The SUN-family protein Sad1 mediates heterochromatin spatial organization through interaction with histone H2A-H2B
Heterochromatin is generally associated with the nuclear periphery, but how the spatial organization of heterochromatin is regulated to ensure...
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General Characteristics of the Sun
In this chapter, we give a brief overview of the general characteristics of the Sun and its activity. The internal structure of the Sun is briefly...
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The Sun
Our Sun is the only star whose surface we can study in detail due to its proximity. Through space missions are also in situ measurements possible.
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The Sun: Dark and Cold
AbstractThis paper makes an attempt to describe the ideas about the Sun that dominated Europe in the 17th–19th centuries.
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The Sun and the Earth
This chapter introduces the Sun and the Earth to the readers, starting from the Big Bang. The solar system is described in detail, with special...
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Identification of nuclear membrane SUN proteins and components associated with wheat fungal stress responses
In eukaryotes, the nuclear membrane that encapsulates genomic DNA is composed of an inner nuclear membrane (INM), an outer nuclear membrane (ONM),...
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Is Inner Source the Next Stage in the Agile Revolution?
Modern business leaders know it is important to be able to work fast, adapt to change, and build on existing solutions. This is especially true of...
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Magnetic Fields on the Sun
This chapter presents a general picture of magnetic fields on the Sun. Magnetic fields on the Sun were first measured in sunspots using the Zeeman...
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Main Characteristics of the Sun
The Sun is the central body of our Solar System. It is a hot rotating gas sphere with a radius of RS = 6.96 × 1010 cm and a mass of...
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Small-scale layered structures at the inner core boundary
The fine-scale seismic features near the inner core boundary (ICB) provide critical insights into the thermal, chemical, and geodynamical...
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Sun Bu’er of China 孫不二 1119–1183
Commemorated as one of Seven Perfected Ones (or Seven Perfected Daoist Masters), Sun Bu’Er’s teachings and writings explore the methodology of “inner...
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A Stellar View of the Sun
This invited memoir looks back on my scientific career that straddles the solar and stellar branches of astrophysics, with sprinklings of historical...
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Propagation of coronal mass ejections from the Sun to the Earth
Coronal mass ejections (CMEs), as they can inject a large amounts of mass and magnetic flux into the interplanetary space, are the primary source of...
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Optimal interplanetary trajectories for Sun-facing ideal diffractive sails
A diffractive sail is a solar sail whose exposed surface is covered by an advanced diffractive metamaterial film with engineered optical properties....
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The Sun, Our Nearest Star
In this chapter, we shall look at the Sun, bearing in mind it is a star on the main sequence. With this approach, it is possible to use the Sun as a...
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Ontogenetic differences in sun and shade galls of Clinodiplosis profusa on Eugenia uniflora leaves and the cytological antioxidant mechanisms in gall cells
The gall-host Eugeni a uniflora (Myrtaceae) is adaptable to different light conditions, enabling leaf production and survival in both sun and shade....
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The Sun and Its Restless Magnetic Field
The permanently changing magnetic field of the Sun is the ultimate driver of the various effects refered to as space weather. This chapter gives an...
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On the Question of Localizing the Birthplaces of Coronal Mass Ejections on the Sun
AbstractThe localization of zones of occurrence of coronal mass ejections (CME) on the Sun in the period from November 2006 to February 2007 was...
