@article{22564,
  abstract     = {It is well known that cities increase air and surface temperatures compared to their rural surroundings, the so-called urban heat island (UHI) effect. However, the associated changes in atmospheric humidity (also known as urban dry island, UDI) and convection triggering remain largely unexplored and it is still unclear how urban modifications of the surface energy budget Influence the diurnal evolution of temperature and humidity in the Atmospheric Boundary Layer
(ABL) and ultimately control the initiation of convective clouds.
Here we quantify the impact of different urban settings and free atmospheric conditions on
UHI, UDI, and convection triggers by means of a zero-order model of the ABL. Specifically, we
derive an approximate solution for urban-rural changes in surface energy fluxes and ABL potential
temperature and humidity and we investigate the crossing between the ABL height and the lifting
condensation level (LCL) which is a proxy for the triggering of convective clouds. We show that
urban areas are generally warmer and drier, thus causing an increase in both ABL and LCL
heights. However, the response of the ABL-LCL crossing to surface conditions is non-linear and
there exists a range of free atmosphere conditions for which changes in imperviousness can
impact convective clouds.},
  author       = {Chiu, Clinton T.F. and Wang, Kai and Paschalis, Athanasios and Erfani, Tohid and Peleg, Nadav and Fatichi, Simone and Theeuwes, Natalie and Manoli, Gabriele},
  issn         = {2212-0955},
  journal      = {Urban Climate},
  keywords     = {Urban heat island, Urban dry island, Boundary layer, Convective clouds, Analytical model},
  publisher    = {Elsevier},
  title        = {{An analytical approximation of urban heat and dry islands and their impact on convection triggering}},
  doi          = {10.1016/j.uclim.2022.101346},
  volume       = {46},
  year         = {2022},
}

@article{11606,
  abstract     = {Context. Our knowledge of the dynamics of stars has undergone a revolution through the simultaneous large amount of high-quality photometric observations collected by space-based asteroseismology and ground-based high-precision spectropolarimetry. They allowed us to probe the internal rotation of stars and their surface magnetism in the whole Hertzsprung-Russell diagram. However, new methods should still be developed to probe the deep magnetic fields in these stars.

Aims. Our goal is to provide seismic diagnoses that allow us to probe the internal magnetism of stars.

Methods. We focused on asymptotic low-frequency gravity modes and high-frequency acoustic modes. Using a first-order perturbative theory, we derived magnetic splittings of their frequencies as explicit functions of stellar parameters.

Results. As in the case of rotation, we show that asymptotic gravity and acoustic modes can allow us to probe the different components of the magnetic field in the cavities in which they propagate. This again demonstrates the high potential of using mixed-modes when this is possible.},
  author       = {Mathis, S. and Bugnet, Lisa Annabelle and Prat, V. and Augustson, K. and Mathur, S. and Garcia, R. A.},
  issn         = {1432-0746},
  journal      = {Astronomy & Astrophysics},
  keywords     = {Space and Planetary Science, Astronomy and Astrophysics, asteroseismology / waves / stars, magnetic field / stars, oscillations / methods, analytical},
  publisher    = {EDP Sciences},
  title        = {{Probing the internal magnetism of stars using asymptotic magneto-asteroseismology}},
  doi          = {10.1051/0004-6361/202039180},
  volume       = {647},
  year         = {2021},
}

@article{12940,
  abstract     = {Desorption electrospray ionization (DESI), easy ambient sonic-spray ionization (EASI) and low-temperature plasma (LTP) ionization are powerful ambient ionization techniques for mass spectrometry. However, every single method has its limitation in terms of polarity and molecular weight of analyte molecules. After the miniaturization of every possible component of the different ion sources, we finally were able to embed two emitters and an ion transfer tubing into a small, hand-held device. The pen-like interface is connected to the mass spectrometer and a separate control unit via a bundle of flexible tubing and cables. The novel device allows the user to ionize an extended range of chemicals by simple switching between DESI, voltage-free EASI, or LTP ionization as well as to freely move the interface over a surface of interest. A mini camera, which is mounted on the tip of the pen, magnifies the desorption area and enables a simple positioning of the pen. The interface was successfully tested using different types of chemicals, pharmaceuticals, and real life samples. Moreover, the combination of optical data from the camera module and chemical data obtained by mass analysis facilitates a novel type of imaging mass spectrometry, which we name “interactive mass spectrometry imaging (IMSI)”.},
  author       = {Meisenbichler, Christina and Kluibenschedl, Florian and Müller, Thomas},
  issn         = {0003-2700},
  journal      = {Analytical Chemistry},
  keywords     = {Analytical Chemistry},
  number       = {21},
  pages        = {14314--14318},
  publisher    = {American Chemical Society},
  title        = {{A 3-in-1 hand-held ambient mass spectrometry interface for identification and 2D localization of chemicals on surfaces}},
  doi          = {10.1021/acs.analchem.0c02615},
  volume       = {92},
  year         = {2020},
}

@article{13383,
  abstract     = {Two novel donor–acceptor Stenhouse adducts (DASAs) featuring the catechol moiety were synthesized and characterized. Both compounds bind strongly to the surfaces of magnetite nanoparticles. An adrenaline-derived DASA renders the particles insoluble in all common solvents, likely because of poor solvation of the zwitterionic isomer generated on the nanoparticle surfaces. Well-soluble nanoparticles were successfully obtained using dopamine-derived DASA equipped with a long alkyl chain. Upon its attachment to nanoparticles, this DASA undergoes an irreversible decoloration reaction owing to the formation of the zwitterionic form. The reaction follows first-order kinetics and proceeds more rapidly on large nanoparticles. Interestingly, decoloration can be suppressed in the presence of free DASA molecules in solution or at high nanoparticle concentrations.},
  author       = {Ahrens, Johannes and Bian, Tong and Vexler, Tom and Klajn, Rafal},
  issn         = {2367-0932},
  journal      = {ChemPhotoChem},
  keywords     = {Organic Chemistry, Physical and Theoretical Chemistry, Analytical Chemistry},
  number       = {5},
  pages        = {230--236},
  publisher    = {Wiley},
  title        = {{Irreversible bleaching of donor-acceptor stenhouse adducts on the surfaces of magnetite nanoparticles}},
  doi          = {10.1002/cptc.201700009},
  volume       = {1},
  year         = {2017},
}