User profiles for J. B. Simon
Jacob B. SimonIowa State University Verified email at iastate.edu Cited by 5025 |
Occult blood screening for colorectal carcinoma: a critical review
JB Simon - Gastroenterology, 1985 - Elsevier
The author reviews the literature on occult blood surveillance for colorectal carcinoma. The
guaiacbased Hemoccult (SmithKline Diagnostics, Sunnyvale, Calif.) test is the most reliable …
guaiacbased Hemoccult (SmithKline Diagnostics, Sunnyvale, Calif.) test is the most reliable …
Athena: a new code for astrophysical MHD
A new code for astrophysical magnetohydrodynamics (MHD) is described. The code has
been designed to be easily extensible for use with static and adaptive mesh refinement. It …
been designed to be easily extensible for use with static and adaptive mesh refinement. It …
Predictive value of the Rome criteria for diagnosing the irritable bowel syndrome
…, WG Paterson, LR DaCosta, AG Groll, JB Simon… - The American journal of …, 1999 - Elsevier
OBJECTIVE: Our aim was to examine the predictive value of the Rome criteria and absence
of so-called “red flags” of clinical practice for diagnosing irritable bowel syndrome. Red flags …
of so-called “red flags” of clinical practice for diagnosing irritable bowel syndrome. Red flags …
Understanding and fostering family resilience
JB Simon, JJ Murphy, SM Smith - The family journal, 2005 - journals.sagepub.com
… Simon is an assistant professor of psychology at the University of Central Arkansas (UCA).
She is a licensed psychologist with years of experience working with children, adolescents, …
She is a licensed psychologist with years of experience working with children, adolescents, …
The mass and size distribution of planetesimals formed by the streaming instability. I. The role of self-gravity
We study the formation of planetesimals in protoplanetary disks from the gravitational collapse
of solid over-densities generated via the streaming instability. To carry out these studies, …
of solid over-densities generated via the streaming instability. To carry out these studies, …
Weak turbulence in the HD 163296 protoplanetary disk revealed by ALMA CO observations
Turbulence can transport angular momentum in protoplanetary disks and influence the growth
and evolution of planets. With spatially and spectrally resolved molecular emission line …
and evolution of planets. With spatially and spectrally resolved molecular emission line …
A three-dimensional view of turbulence: constraints on turbulent motions in the HD 163296 protoplanetary disk using DCO+
…, AM Hughes, SC Rose, JB Simon… - The Astrophysical …, 2017 - iopscience.iop.org
Gas kinematics are an important part of the planet formation process. Turbulence influences
planetesimal growth and migration from the scale of submicron dust grains through gas-…
planetesimal growth and migration from the scale of submicron dust grains through gas-…
Measuring turbulent motion in planet-forming disks with ALMA: a detection around DM Tau and nondetections around MWC 480 and V4046 Sgr
Turbulence is a crucial factor in many models of planet formation, but it has only been directly
constrained among a small number of planet-forming disks. Building on the upper limits on …
constrained among a small number of planet-forming disks. Building on the upper limits on …
Turbulence in the TW Hya disk
Turbulence is a fundamental parameter in models of grain growth during the early stages of
planet formation. As such, observational constraints on its magnitude are crucial. Here we …
planet formation. As such, observational constraints on its magnitude are crucial. Here we …
Emergent mesoscale phenomena in magnetized accretion disc turbulence
JB Simon, K Beckwith… - Monthly Notices of the …, 2012 - academic.oup.com
We study how the structure and variability of magnetohydrodynamic (MHD) turbulence in
accretion discs converge with domain size. Our results are based on a series of vertically …
accretion discs converge with domain size. Our results are based on a series of vertically …